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I am maintaining an N2a cell line and I can see black dots that for the most part seem non-moving (a few seem to exhibit Brownian motion) but I am not sure if it's bacterial contamination, cellular debris or possibly something from the serum. The pictures are after I have washed the cells. Thank you for the help.
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@Neda Kaveh the images I uploaded were after they were left for 4 days and I didn't see much difference on day 5, the only difference was that I had more floating cells since they were overconfluent. I also checked the media and PBS and they were fine and I typically leave my media at 37 degrees for 30 mins or more before passaging
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As these images shown, black dots seem adherent on my cell ,can be slightly observed under 400× magnification.They cannot be removed by PBS washing or medium repalcement ,and antibiotics ,including penicillin, streptomycin, gentamycin, neomycin , ciproflaxin and purchased myoplasma removing reagents are useless to them. These dots only exist on the cells and could be observed moving under 400× sight ,I am not sure if it is brownian motion. Colleagues in the same lab using same batch of serum or medium never find this phenomenon but we cultured different cells .
I m sure it is not bacteria contamination ,for no colony found on LB plate after 48h of incubation at 37℃ with cultured medium added on. If there 's possible that it is mycoplasma , which is resistant to mycoplasma removing reagents.
Could anybody give me some advice? really appreciate.
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It is most probably mycoplasma contamination..
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Electrical circuits for different experiments e.g Brownian motion, Hystesis Law and etc
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Yes
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It is well known that the Brownian motion and the related Wiener process have many different applications in different fields.
Roughly speaking, the Wiener process can be thought of as a function of two variables W(x, t).
Note that for each fixed x point W(x, t) = f(t) is a continuous function, often called a trajectory.
Various properties of such trajectories are known, one of them is that the function f(t) is not a function of finite variation in the Jordan sense, but f(t) is known to be a function of finite variation in Wiener sense, for some number p>1.
In the literature that I have access to, the connection between finite variation in the Wiener sense and Brownian motion ends with this last result.
I wonder what role the number p plays. Does the number p have any interpretation in physics, economics, or any other field?
I will be grateful if someone can refer to the literature that describes such interpretations of the number p.
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Bounded quadratic variation of a Brownian motion. where the supremum is taken over all possible partitions Π of the interval [0,T ] for all n. A function f is defined to have bounded variation if its total variation is finite. ... Brownian motion is almost surely nowhere differentiable.
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Given that non-spherical particles (e.g., rods) will exhibit optical anisotropy due to their continuous rotational Brownian motion, and even if the scattering signal is concurrently obtained and then combined from multiple detection angles (MADLS), how reliable are the size measurements obtained from DLS/MADLS for non-spherical particles?
I can see how MADLS size measurements can be reasonable if the non-spherical particles do not change their orientation with time. But since rotational Brownian motion in unavoidable, I am not sure how/if that can be factored in the measurement and/or data processing.
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Dear Omar!
Reliable measurements of non-spherical particles by the dynamic light scattering method are possible only when depolarized light is recorded. In this case, you can separate the contributions of translational and rotational diffusion to the autocorrelation function. A description of such measurements can be found in the article by Robert Pecora (https://www.researchgate.net/publication/226509433_Dynamic_Light_Scattering_Measurement_of_Nanometer_Particles_in_Liquids). For rod-shaped particles, one can try DLS measurements in oriented systems. That is, an external field (for example, an electric field) to orient the particles in a certain direction and determine the size as in the classical DLS. Perhaps, it will be possible to fix the difference, since for the rod the coefficients of translational diffusion are very different along and across the long axis, and rotational diffusion will be excluded (the axes of the particles are aligned in the same direction).
Good luck!
Best regards, Constantine Yerin
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The particles are Nanoparticles. How from their light scattering we can calculate their size
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Particle size as a function of Brownian motion is determined by dynamic light scattering. If the particles are solid, they get approximately constant sizes. If the particles are from "soft matter", then difficulties arise. For measuring the size of surfactant micelles, see
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Hello,
Is it possible to observe Brownian motion of particles with a light microscope at 40X? I am asking for reasons relating to mammalian cell culture.
Thank you.
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The botanist Robert Brown, who is usually credited with the discovery of Brownian motion, discovered it while studying pollen grains of a plant suspended in water under a light microscope in 1827.
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Hello,
Wondering if there are any physicists that can explain (very simply as I am a chem eng) whether a charged particle would move faster or slower through water than an uncharged particle. Perhaps this is somewhat explained by brownian motion?
For example, if I have an ionic solution (e.g. salt) would the particles move faster than a neutral solution or similar molecular weight? Or more simply would Na+ move more quickly than Na. Does the charge (pos vs neg) matter?
If you know any pubs that explain this that would be great too as everything I find is more looking at charged particles moving in an electric feild.
Thank you.
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It's not possible to give an unambiguous answer. A neutral particle is made up of charged particles anyway. Water has an electrical dipole moment so it's the coupling between this dipole moment and the particle that matters. A neutral particle can only couple to the dipole moment of water through its dipole moment (if it doesn't vanish, as well-in which case it's the quadrupole moment that matters); an electrically charged particle can couple to the individual constituents of the dipole. So it can lose energy more easily and therefore one might say that it will be slower than a neutral particle that can't lose energy as easily, since it interacts less strongly with water molecules.
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In the Dynamic Light Scattering (DLS) method, the exponential decrease of the autocorrelation function means the Brownian motion of particles in the dispersant. If it does not decrease exponentially (if it follows polynomial, zigzag, or linear manner), then what does it indicate regarding the particle motion?
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There are a number of factors and effects that can cause an irregular autocorrelation function to be measured.
In general a non exponential decay is caused by either non brownian motion being detected, or the average scattering intensity changing during the measurement. There are several potential causes for either of these.
The following webinar discusses how to interpret DLS data and may be of interest.
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I have done a numerical simulation of a nanofluid in a microchannel heat sink using Al2O3-water nanofluid. In this simulation, I used a single-phase methodology since I have all the thermophysical properties of the nanofluids from experimental data.
Is it still possible to quantify the effect of Brownian motion and Thermophoresis on my microchannel system? If yes, what do I need to do?
Thank you for your help
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For your purpose you sould use the 2 phase nanofluid model
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I am doing an experiment with colloidal solution of nanoparticles and would like to measure the Brownian motion velocity of these particles. Can I do it experimentally?
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Prajal Chettri You get the diffusion coefficients directly and they can be plotted out - it's these that are transformed to PSD. Indeed in the Stokes-Einstein relationship there's a direct linear relation between hydrodynamic size and diffusion coefficient. so the plots will look identical (except that the x-axis will be different).
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In probability theory, fractional Brownian motion (fBm), also called a fractal Brownian motion, is a generalization of Brownian motion. Unlike classical Brownian motion, the increments of fBm need not be independent. fBm is a continuous-time Gaussian process BH(t) on [0, T], that starts at zero, has expectation zero for all t in [0, T],
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Thanks for your useful answers.
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Besides temperature, particle size, and fluid viscosity, what other factors affect Brownian motion in a suspension?
Let's say I have a suspension and wish to increase the Brownian movement of its particles, is there a way I can do so without having to increase its temperature? What other things can I do to the suspension to achieve this (e.g. could I change the surface charges of the particles? Could I sonicate the suspension? Could I run an electric current through the suspension? Could I run a magnetic field around the suspension?)
Thank you.
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Apparently, you mean only external influences upon Brownian motion. The acceleration of the Brownian motion of particles in suspension is also influenced by factors such as shape (for example, if the particles have a long shape, then the translational Brownian motion is also superimposed by a rotational movement that increases the probability of collision of such particles; etc.); heterogeneity (in the sense of heterogeneity of the material); proportion of different particle sizes (depending on the characteristics of the suspension, different optimal proportions of particles occur; by the way, finding the optimal proportion of heterogeneous particle sizes under fixed other characteristics and conditions is a very interesting mathematical problem).
The above-listed factors, obviously, are not external factors of influence, – they are "internal" factors.
Further, from the external factors listed by you, the last two factors influencing the acceleration of Brownian motion.
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Raum und zeit, space and time, were united by Minkowski in 1908 to elucidate Einstein’s special relativity. Time flows. Can the idea of the fourth dimension be generalized to any system that includes three dimensional space and one dimensional flow? One dimensional flow can include molecular motion, photons, wind eddies, Brownian motion.
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The so-called “spacetime”, the fundamental basis of GRT is an abstract and esoteric geometrical/mathematical construct; supposedly with impossible physical, mechanical, metric etc. properties. This is a theory of mathematics but not a theory of physics!
For a more scientific and philosophical view of space and time please the following:
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Dear colleagues.
For the fungi-air system, I have difficulty defining the range of values that the molecular diffusion coefficient $D$ can assume. For fungi with 20-30 microns, ie 20-30 x 10^(- 6) m, some texts suggest the range from D=0.0001 m^2/h to D=0.1 m^2/h, but these values seem very low to me. Please, if anyone has measures or texts to suggest, I appreciate it.
Regards,
Dr. Paulo Natti
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Fungi are not molecules, they are medium size airborne particles. You can't apply the term "molecular diffusion coefficient" for such particles. You may need to know the sedimentation rate.
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I understand that the Hurst exponent of the Gaussian white noise is equivalent to 0 theoretically, because of the definition of fractional Brownian motions, fBms.
Why do some papers say that the exponent is -0.5, not 0?
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I answer a long time after your question, Takumi Sase, but in case you are still working on it:
- The Hurst exponent of the standard Brownian motion (Bm) is 0.5. One can define fractional Brownian motions (fBm) of Hurst exponent H (in (0,1)). If H>0.5, the fBm is a fractional integral of order H-0.5 of a Bm. If H<0.5, the fBm is a fractional derivative of order 0.5-H of a Bm.
- The Bm is an integral of white noises (increments of a Bm are iid Gaussian variables, these increments are the white noise), so we couldsee the white noise as a derivative of Bm. The standard derivative is also "a fractional derivative of order 1". So, consistently with the previous paragraph, one could say that the Hurst exponent of the white noise is 0.5-1=-0.5.
- Alternatively, if one considers the white noise process X_t, the process is distributed in the same way at every time: X_t has the same distribution as X_s. Following Mandelbrot's definition of self-similarity (Y is H-self-similar, with H the Hurst exponent, if Y_t has the same distribution as (c^{-H})Y_{ct}), one concludes that X has a Hurst exponent equal to zero.
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Why did Galileo build his analysis of the strength of animal bone for an animal of increased weight from a scaling standpoint and not a dimensional standpoint? The scaling he used is induced by dimension? Did dimensional capacity raise issues that seemed best avoided? Did the principle of dimensional capacity raise issues irrelevant for the new science of strength of materials? The dimensional standpoint seems involved in metabolic scaling, Brownian motion, and dark energy (expanding space), the cosmic scale factor, among other modern questions. Hence the question, implied in the article:
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Galileo never thought that gravitation were going to permit a change of scale in the Universe and even he thought the inverse employing the effect between weight and bones resistance.
At present what we have is a map of what "could be the distribution of the dark matter in our Universe" using weak gravitational lensing. The scale changes don't play any role in this representations at all. The most important part corresponds to have a cross-correlated mass map based with maps of galaxy and cluster samples in the same dataset looking for the statistical significance. This is interesting but without any relationship with an scale physical consequence that were not known: on what scales are matter and geometry coupled by Einstein’s equations?. In standard cosmology, the FLRW metric is assumed to exactly describe the average growth of the Universe on arbitrarily large scales. However, in a generally inhomogeneous universe as described in timescape cosmology, this is no longer the case.
Dark matter follows to be nothing more than an hypothesis and what is a problem is if our gravitational models are enough for explaining the whole Universe making a comparition of such scale with ours.
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Has anyone come across bacterial contamination which is very slow growing? only growing to cover the flask over 2-3 weeks (of media not changed)? Also not changing the pH of the medium, nor turning cloudy or yellow. Cells are still growing not dying. At first i thought it was just cell debris until i removed medium into a flask without cells and watched over weeks as the dots went from just afew per field of view to totally covering the flask. The dots, upon staring at them, move with brownian motion. I see in my FBS straight from the aliquot (2 different aliquot dates too). I have decontaminated incubators water bath, changed tips in pipette gun, etc. If this is coming from the FBS it just keeps turning up. Will preciptates from FBS jiggle around like brownian motion?
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Please go through the reference given below . This may help you to understand the problem you are facing
Biologicals. 2010 Mar; 38(2): 273–277.
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Kindly answer this question so that I can understand better about ( relationship between Brownian motion and temperature gradient on enhancement thermal conductivity) and what is the meaning of ( temperature gradient) in nanofluid ?
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Dear Researchers,
Have a nice weekend with your family....
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Hello every body,
I have got a set of GPS data containing the hourly locations of 74 terrestrial animals during the study period. Currently, I am looking over disparate models of movement modelings like BBMM. I need to study the interaction and movement pattern of each individual animal.
In addition, I will use Python for the implementation of the model.
Which model do you recommend?
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Hi, it appears that no one has really answered your question, so I am going to take a stab at it and hopefully it helps. If you are using Esri products in the Geoprocessing tools there are the Spatial Analyst and Tracking Analyst extensions that are really helpful. You can build a model, through modeling building and test how it works. They do require some level of knowledge with ArcGIS and GIS. However, there are online tutorials for ArcGIS extensions, and YouTube videos, for free. I have seen in other forums people suggesting Hawths’ tool for spatial ecology, but I am not familiar with that software at all that I am aware of.
Tracking analysis
Spatial analysis
or if you read enough which most college students do check out the choices in YouTube videos
Spatial analysis YouTube
Tracking Analysis YouTube
Animal movement article with resources
Also: a book is out on explaining Modeling suitability, movement and interaction
I hope this helps, Good luck with your project.
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Hello,
Recently I performed lentiviral transduction on several cell lines. On day one with the lentivirus, I observed black aggregates moving (dancing, vibrating) around my cells. These are only in cells to which I added virus.
When I harvested my lentivirus in the supernatant of my packaging cell line, I spun the supernatant (3000RPM for 15 minutes) to remove cellular debris, filtered it with a 450nm sterile filter, and then froze it at -80C. These steps should have removed bacteria, correct? Moreover, the aggregates are resistant to the 1% Pen/Strep in my culture media. They do not turn the media turbid, and they never seem to reach log phase.
Could I be seeing the virus itself?
Can lentiviruses form visible aggregates?
Could these be abiotic aggregates exerting Brownian motion?
I have seen this phenomenon before and as of now, no one has given me a satisfactory answer regarding the identity of the dots.
Thank you.
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It's not advisable to filter lentivirus with a 0.22um filter - you'll lose some. That's why a 0.45um filter is generally recommended.
There are companies that will analyse cells and culture media for you to look for Mycoplasma and many other contaminants - that's probably the best way to know for sure.
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There are reasons to think so, if one connects theory for a variety of phenomena.
First there was a novel explanation for metabolism scaling by a 3/4 power of mass (Kleiber’s Law). That explanation emerged beginning in 2008 based on an animal’s circulatory system scaling by a 4/3 exponent of circulatory system volume. Metabolism scales by an inverse exponent, by a 3/4 power to maintain animal body temperature. In effect the entropy of the circulatory system is 4/3 the entropy of tissue supplied by the circulatory system.
The same 4/3 scaling of entropy occurs in an intermediate step of Stefan’s Law (1879); the derivation was worked out by Boltzmann but the most accessible derivation is that of Planck in his text book on heat. Since Stefan’s Law applies to black body radiation and the universe can be considered in the large as a black body cavity, the involvement of Stefan’s Law is, at least, intriguing.
In 1859 and 1860, Rudolf Clausius gave a demonstration in connection with the kinetics of gas molecules that in effect says that lengths stretch by 4/3 in stationary three dimensional space compared to four dimensional space with motion. If Clausius’s derivation is modified to apply to photons instead of gas molecules, then 3 dim space itself would stretch by 4/3 relative to 4 dim space consisting of 3 dim space + light motion.
In 1926, Lewis Fry Richardson measured that wind eddies scale by 4/3, an observation similar to that of Clausius in 1859 and 1860. In 1941, Andrei Kolmogorov provided mathematical derivations.
In 2000 or so, the fractal envelope of Brownian motion was determined using sophisticated mathematics (stochastic Lowner evolution) to be 4/3.
Common mathematics appears to connect all of the foregoing. That suggests that the 4/3 ratio arises, for comparable circumstances, as a universal law.
In other words, by connecting different phenomena that all relate to 4/3 scaling, one can infer a general law.
Since 4/3 scaling appears to be a general law, it should not be surprising if it applies at a cosmological scale.
It is therefore intriguing that the ratio of energy densities for Omega_r / Omega_M for r radiation and M matter, has been measured at about 0.70 / 0.30. This is very close to the ratio of cosmological energy densities that would result from 4/3 scaling for energy E: E/ (1)^3 : E / (4/3)^3 = 4^3 / 3^3 = 0.7033 / 0.2967. In fact the survey of type 1A supernova by Betoule et al in 2014 measured Omega_M as 0.295 which is exceptionally close indeed to what theory suggests.
It is moreover interesting that the 1998 observations inferred that type 1A supernovae were about 10 to 15% farther away than expected based on luminosity about 3/4 as bright as would be expected for a flat universe. But 3/4 luminosity is equivalent to being 4/3 as far away if two reference frames, one 3 dim and the other 4 dim, are assumed consistent with 4/3 scaling. The 10% to 15% estimates were based on the implicit assumption that looking out into the universe looks out on a single 3 dim space, not two reference frames of 3 and 4 dim.
So. Do the dots connect?
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Why did the wrong "entropy" appear ?
In summary , this was due to the following two reasons:
1) Physically, people didn't know Q=f(P, V, T).
2) Mathematically, people didn't know AΔB couldn‘t become AdB directely .
If people knew any one of them, the mistake of entropy would not happen in history.
Please read my paper and those answers of the questions related to my paper in my Projects.
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In DLS method, the time dependence of scattered light intensity is used to obtain autocorrelation function (usually characterized by about 100 points). Then this function is fitted, and the inflection point of the fit corresponds to the characteristic time of the process in the sample. If we assume that this process is the Brownian motion of particles, then we can calculate characteristic size of these particles (regarded as hydrodynamic size; assuming spherical particles, and taking into account viscosity and refractive index of the medium).
Is it possible to achieve the estimate of this particle size with accuracy better than 1 nm for particles, say, of 10 nm? I suspect that it should be inherently limited by accuracy of the fit for the autocorrelation function.
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The correlation plot is an exponential decay and thus is very low resolution (only 2 parameters needed to define it), so the '100 points' in your commentary doesn't imply more accuracy or precision - a better fit doesn't necessarily result. We also note that size standards in the < 100 nm range tend to be characterized by electron microscopy, so there is not a like-for-like comparison. We also note that the approximate size of a hydrogen atom is 73 pm (or about 0.07 nm), so the best we would hope to achieve would be quoting to +/- 0.1 nm. However, DLS measurements of materials like sucrose (sub-nm) by DLS are supported by other molecular data. See the attached.
We also have to be aware that we're relating a diffusion coefficient to size (via Stokes-Einstein) and thus covering stabilizers and surfactants are factored into the hydrodynamic size. And 'size' is an ambiguous term for irregular particles.....SAXS or electron microscopy shows the electron-dense region of the particle and thus will not consider or 'see' the adsorbed layers. I think 10 +/- 0.1 nm is probably the best we could hope to achieve (with all the notes and caveats above). However, we must be positive about the DLS ensemble technique - how else can we get information from billions of particles simultaneously with great sensitivity in the intensity distribution to the presence of tiny amounts of aggregate.
The certificate for the RM8011 standard from NIST is enlightening in this respect.
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The fundamental solution to the Diffusion Equation in one dimension is
c(x, t)=1/(4(pi)Dt)^1/2 e^( - (x - xo)^2/4Dt) ,
where D is the Diffusion constant of the diffusing particle, t is the time, x is the position along the x-axis, and xo is the initial position of the diffusing particle.
In the above equation, the center (mean) of the pulse is taken to be stationary at x = xo.
If the pulse were to drift in one direction along the x axis so that its center (mean) moved with velocity v to the right, the moving pulse would be expressed mathematically as
c(x, t)=1/(4(pi)Dt)^1/2 e^( - (x - vt)^2/4Dt) ,
where v is the velocity of the center (mean) of the pulse along the x-axis.
However, if the center (mean) of the pulse were moving randomly, so that it undergoes Brownian Motion, how would c(x, t) be expressed so that it could be evaluated (numerically) for each given (x, t) pair?
Any information related to the answer of this question would be greatly appreciated.
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Hi,
I don't have any reference to give you, but, as I understand your question, you have two independent diffusion processes:
* There is a particle (2) diffusing with constant D_2 with respect to a medium.
* There is a medium (1) diffusing with constant D_1 with respect to the desired frame of reference (0).
* Let x_21 be the coordinate of the particle w.r.t. the medium.
* Let x_10 be the coordinate of the medium w.r.t. the frame of reference.
* The probability density function (PDF) for the particle w.r.t. the medium is
c_21(x_21, t)=1/(4(pi)D_2t)^1/2 e^( - (x_21)^2/4D_2t)
* The PDF for the medium w.r.t. the frame of refernce is
c_10(x_10, t)=1/(4(pi)D_1t)^1/2 e^( - (x_10)^2/4D_1t)
* The position of the particle w.r.t. the frame of reference is
x = x_21 + x_10 => x_10 = x - x_21
* If the diffusion processes are independent, we have
c(x, t) = integral c_21(x_21, t) * c_10(x - x_21, t) d x_21,
with the integral taken of the domain of x_21.
I don't know if there is an analytical solution to this convolution, but you can easily find out with Maple/Mathematica/Matlab.
Good luck,
/Stefan
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I'm experimenting the modeling/simulation of some processes using the Perlin noise, of which I've gain only some basic understandings. According to this article (https://flafla2.github.io/2014/08/09/perlinnoise.html), the gradient vectors control the distribution of the resultant map (I'm only concerned with 2D maps), if the 4 corner gradient vectors converge, there will be a region of local maximum, and vice versa. So if I want to have some inference on the distribution, I believe these vectors are the way to go. My question is how to bind the orientations of the 4-corner-vectors of some selected cells with the probability of there being an local maximum? Suppose for some cells, I want there to be near-permanent positives. And for some other cells, the probability of seeing a local maximum/minimum is controlled by observational values.
Could anyone give me some hints how to handle this?
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It turns out that you can invert a Perlin noise perfectly rather easily, if the input is a Perlin itself. Or fit a set of gradient vectors in a least squares sense if the input is not generated from a Perlin procedure. Then the inverted gradients can be used to build distributions.
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I would use the variance in the Brownian motion using equipartition theorem to calculate the trap stiffness, but I could not understand how I choose the points that is representative to be used for the calculation,
shall I use the just after calibration of position detector, or the straight-line on which beads are trapped by light before I start the real experiment.
As both values of variance differs and the difference is big enough to create different results (SD=2.1, 5.8 nm).
Does difference between these values mean something wrong in the our optical tweezer
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Why do not use the power spectrum method (PSD) to get both stiffness (k) and sensitivity(S)?
The PSD is calculated by Fourier transforming the QPD signal in Volts and is fitted with a lorentzian function to determine two constants: the plateau and the corner frequency, which define S and k.
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Do you know of any interactive apps that allow users to setup simple 2D simulations, such as:
- repulsive gas,
- liquids,
- brownian motion,
- polymer solutions,
- etc.
?
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Although EspressoMD also looks inviting, I'm currently going with OpenMM. This one has a fairly good userguide to start creating customised forcefields, defined in XML. Have made a simple set of CG-particles.
NB for future readers: As of writing, openMM matches molecule topologies to forcefield descriptions by matching bond networks with correct element names.
Docs:
Forums:
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dX= u dt + s dw
  • u is referring to drift
  • s(sigma) is referring to volatility
suppose I have data for 3 years. how can I estimate (u and s)
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Hi,
You can stick to maximum likelihood estimation, and depending on the requirements of your project (speed,limited number of data entries etc. etc.) you can then adjust or search for a faster solution.
I would recommend to check the sde package in R and search for articles limilar to this one: https://arxiv.org/pdf/1408.2441.pdf
Best regards,
Stan
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These are examples of the 4/3 law so called by Hunt 1998. Lewis Fry Richardson’s 1926 measurements of wind eddies and Kolmogorov’s 1941 proof. John James Waterston’s 1845 on a gravitating plane. Clausius 1858 on 3/4 mean path lengths. Boltzmann’s 1884 derivation of Stefan’s law. Kleiber’s 3/4 metabolic scaling. The 4/3 fractal envelope of Brownian motion in Lawler 2001. Brittin and Gamow 1961 on photosynthesis, an implicit reference. In cosmology energy density varies with distance as 1/a^3 for matter and 1/a^4 for radiation. Jafar and Shamai 2007, perhaps, on cell phone transmission towers. The 4/3 law has two guises. First, a system with 4 dimensions has 4/3 the degrees of freedom of one with 3 dimensions. Second, lengths in a 4 dimensional system are 4/3 longer in the 3 dimensional system. The 4/3 law may account for dark energy.
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Dear Robert, in Newton-like cooling law models, some authors proposed an exponent = 4/3 for the difference of Temperatures (see attached paper, page 21). Gianluca
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we have some cost data of the equipment. about 3 years.
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try using adaptive bayesian forecasting (ref Springer---Bayesian Forecasting and Dynamic Models
Authors: West, Mike, Harrison, Jeff )
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Often in astrodynamics we need conducting a high order integration of orbits in higly pertubed dynamics (the n-body problem augmented by the solar radiation pressure, J2, atmosphere, low-thrust, etc.). Some problems that I investigate require precise trajectory propagating. Does anybody know a very precise method of order, say, 30, 35, 40?
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Hi, the precision of the integration can be achieved by any classical integrator (ode45, dopri8, etc...) with variable step. On output  you will obtain the relative and absolute precisions you put on entry. When increasing the order of the integrator  more calculus will be done at each step but the number of steps required to achieve a given precision will be lower. This is the only difference. Thus, if your problem is not stiff you can use any classical ode solver whatever the complexity of your dynamics.
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Particles will show random motion under a microscope. Is there an approximate equation to describe the mean translation velocity as a function of experimental parameters such as size, viscosity and temperature? Thanks!
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The paper that Yashawantha shares does not give an answer to this question, but does discuss the velocity of sedimentation, which is a process which should be considered in verifying that a dispersed system is stable. 
In terms of describing the Brownian motion of particles in suspension, MSD is generally rather than velocity as it makes sense to consider how far we may expect a particle to have moved by random events over time. Root mean square velocity may be calculated in describing the dynamics of gas particles, but there the dynamics are different. 
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I am trying to estimate the 3D position of a point in space by measuring acceleration.This can easily be done by computing the integral of the integral over time of each component of the acceleration vector.
The question is how to statistically characterize the noise. If I assume uncorrelated zero-mean Gaussian noise on the acceleration, the error on the velocity will be a zero-mean Brownian motion, and the error on the position will be the integral of a Brownian motion.
Do anyone know any literature on how to statistically characterize the integral of Brownian motion?
I thank you in advance
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Using only accelerometers will not bring you anywhere. First you should correct for gravity, then the double integration will explode any inaccuracy. The solution is to combine accelerometers with other sensors, like gyroscopes and magnetic sensors, maybe a GPS receiver.
Such a device 'Xsens' is commercially available.
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If the value of Hurst exponent is in the range of 0.55-0.65, then can theoretically random walk hypothesis be strongly rejected? As literature reports studies where time series having Fractional Brownian Motion correspond to higher ( in the range of 0.85-0.95) Hurst exponent values. Similarly for anti persistent pattern if Hurst Exponent Value is in range of 0.40-0.45 what can be inferred?
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 Hi, perhaps, H=0.54 implies that the signal follows only the Wiener process, namly standard Brownian motion. So, I think you should do surrogate test.
I hope my suggestion will help you. :)
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Bio-molecular system interaction by tiny field from UV how problematic for its thermal stress development?
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@Bablu K. Ghosh
Thank you for the references. The missing part of all these studies is indeed an absence of the formal analysis of the interaction of electromagnetic waves with the biological matter. An appropriate assessment should be performed using the Maxwell equations. You can find quite good discussion of the relevant methodology in
I hope that this direction of research could be accommodated in your study.
With my best regards,
Janusz Pudykiewicz
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turbulent flow
I am using Brownian motion dynamics in my equation.two particles are connected through linear spring.I want to generate random force for these two particles using Gaussian distribution.Since this is three dimensional problem so it has 3 independent components.in order to get different value at each run i need to use different seed at each time step.my question is that how we can get different seed for each run?
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From your question I gather that you are not an expert in (pseudo)random numbers yet. If I am right, a good introduction is in the book "Numerical Recipees" (for any computer language) or in the book of Daan Frenkel and Berend Smit. There are more sources, but these two are easily accessible.The best I read to date is chapter 3 of Donald Knuth's volume 2: "Seminumerical algorithms" from the series "The Art of Computer Programming".
An answer to your question might be available at random.org where "real" random numbers are available. Whether that is sufficient for your purpose needs to be checked so you will have to do statistical tests to prove the correctness of your results. Some of such tests are described in the mentioned books.
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Nanoparticles dispersed in liquid are known to undergo Brownian motion. I feel that from time to time, two individual nanoparticles can come close enough to spaces of 1-3 nm and form transient dimers, before separating. I was wondering if there is any method to model this interaction time in terms of the concentration of nanoparticle,distance between the nanoparticles, solvent viscosity and solution temperature. Can anyone please suggest me where I should start looking for the same?
Regards
Rifat Kamarudheen 
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and Chapter 2 by Zhang in Nanomaterial: Impacts on Cell Biology and Medicine
(Most of what you need can be viewed via Google Books here without buying the book - you'll find the references to Smoluchowski and aggregation kinetics)
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At first the viscosity is following simple trend i.e viscosity is decreased when temperature is increased which might happen due to increases in Brownian motion of droplets.
However beyond a certain temperature limit viscosity is increasing. Upon physical identification the emulsion seems to be stable at higher temperature.
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Dear Neetish,
I have no paper for your system, I do not know in detail, however, problem of flocculation goes back to the general basic balance of attractive and repulsive forces, which can be quite complex. If attractive forces dominate structure builds up leading to increased viscosity.
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Hi,
I work with MDCKs. Typically, we put Pen/Strep into our media. Recently, one of my transfections has been determined by the lab to be contaminated. This has made me worried. How do you tell if you have contamination? Obviously, I plan to do a Mycoplasma test on my cells since those are basically invisible. But what other ways can I tell?
The media does turn yellow after the cells have been in it for about two days (assuming I do not change it). But I'm pretty sure that's just exhaustion of media. I haven't observed any slowed growth. It takes about 2 days from thawing to confluence or from split to confluence. Their morphology hasn't altered, either. They look fibroblastic when growing and then nestle into nice little cobblestones when done.
I do see little black irregular dots oscillating at 40x. However, it seems like this is just Brownian motion as they don't really go in a specific direction. And there aren't many, even after two days with no media changes. There's probably one for every two cells? If I did see something swimming/darting around, I'd toss everything immediately. The lab says it isn't contamination.
Throwing the cells into wells has them all turn the same color at the same time at the same rate, too!
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Hi Colin,
Contamination is the most challenging and commonly faced problem for all cell culturists. For identification of contamination, i.e. to be sure if at all there is something contaminating your cell culture you may try these:
1. Try not to discard the spent media but keep it in a plate (may be in a 60mm one), if the media turns yellow or cloudy even then, you know it is contamination! To determine what the contaminating organism is, microscopy is the best way.
2. Fix the cells and stain with DAPI. If you see DAPI staining in small dots outside nucleus, you know that it is staining the DNA of your contaminant.
3. Trypan Blue staining showing small dots with dark outline and lighter inner space indicates presence of contaminants.
4. For simple light microscopy, under 40X magnification, if you see black dots stuck on the plate which doesn't seem to go even if you change plate daily, and also has some kind of brownian motion, its bacterial cells that you are looking at.
To prevent contamination-
1. If you have already identified it to be mycoplasma, then there are many preventive measures which might help you. Like you can use 0.1 micron filter to filter sterilize your media and other stuffs of cell culture.
2. I heard Plasmocin from Invivogen is very effective to combat mycoplasma infection. You can follow the link for further information.
3. Also, even though your cells look healthy, their morphology or growth rate doesn't change, appearance of black dots indicate that you need to check for contamination. 
4. Colour change of phenol red is not sufficient enough to determine the presence of contaminant, as rate of colour change depends on the confluency and number of cells seeded. 
Hope it helps!
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Imagine a very small particle in air (I call it Brownian particle, maybe its not correct). This Brownian particle is "dances" (or oscillates) in air due to air molecules. BUT! When this particle is oscillates it should create some wave around himself. Because during oscillating the particle strikes air molecules and we can imagine this particle sound source. I know that this oscillating is not coherent but there is some oscillating and it should be some wave around this oscillating Brownian particle. Am I right? I searched any information about this wave but I cant find. I liken these waves to pilot-waves of walking droplet.
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Hi
I believe all boils down to fundamental assumptions on length and time scales when formulating the wave equation. Simply put, you state a case where you ignore the micro and focus on the macro properties.
An acoustic wave propagates in a medium that can be described by gross quantities rather than at the molecular level. For things to meet this assumption the average gas particles need to bump into each other quite frequently. If memory serves me correctly, I believe for air at 20 c and ambient static pressure, the average particle contact time is in the ballpark 1E-8s. This would not be the case at near vacuum conditions.
I suggest you look at some books starting from the very fundamentals to better answer your questions, e.g. this excellent book
or this one by A.D. Pierce
If your interest lies in molecular vibration, I can tell you that the N2 molecule vibrates at one of its molecular natural frequencies and may affect acoustic properties. This is so when the N2 molecular vibration is taken up by an adsorber, such as active coal. The N2 molecule then sticks to the surface of the active coal and the loss of molecular vibration energy can be seen as acoustic absorption. The effect is visible up to 80-100 Hz for ordinary air and the phenomenon has been exploited in loudspeakers. http://kef.com/html/en/innovation/ace/index.html
Note the difference between the adsorber (active coal) providing acoustic absorption (damping, i.e. a conversion from vibration to heat).
Sincerely
Claes
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I am looking for a simple software that is able to track single and individual (dilute) particles and to retrieve diffusion coefficient values out of it.
The system is the simplest possible: micron-sized particles undergoing 3D diffusion in water or 2D brownian motion when attached to a planar surface.
1) What parameters are important for recording a time lapse?
2) Any suggested (user friendly) software for non experts?
3) How does one retrieve diffusion coefficient values from the tracks?
Thank you in advance,
Rafael
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Rafael,
I am answering your questions 1 and 3 based on my past imaging experience:
1) What parameters are important for recording a time lapse?
If you use bright field, then you record the positions vs. time of your particles (Xi, Yi, ti) for 2D diffusion or (Xi, Yi, Zi, ti) for 3D diffusion. If you use fluorescence then you record peak intensity spots vs time associated with the particles. Since your particles are micron sized you can go with either (if the particles are fluorescent); otherwise you go with bright field using a 100x objective of large numerical aperture NA=1.0-1.4 for good resolution).
3) How does one retrieve diffusion coefficient values from the tracks?
You collect sufficient mean square displacements (MSD) vs time lapse delta(t) for some 100-500 particles until the histogram appears having a smooth contour, and then calculate the average diffusion coefficient D for your particles based on MSD=4D*delta(t) for 2D diffusion or MSD=6D*delta(t) for 3D diffusion.
Here is a trivial paper of mine on the topic many years back, FYI:
Hope that helps.
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I am working on the natural convection in nanofluids in a square cavity in the temperature range of 30 - 90 degree Celsius. Which type of thermocouples will be best suited to measure the temperature of nanofluids by considering the fluctuation in temperature due to the Brownian motion of nanoparticles. 
Can I use the T-type thermocouples? 
What will be the effect of thermocouple's tip diameter on the measurement of temperature?
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Thanks once again Mr. Jose...
The thermocouples, which I am using, have the bead size of 1 - 2 mm, while the Brownian velocity of nanoparticles is about the order of manometers. Whether it is ok to use such type of thermocouples at nanoscale?
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to support chaos theory in brownian motion.
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I am trying to figure out why the output of fractional Brownian motion as described by Richard Voss (Random fractal forgeries. In: Fundamental Algorithms for Computer Graphics, R. A. Earnshaw (eds.). Springer-Verlag, Berlin. 805-835. ISBN-13: 978-3-540-54397-8) is characterized by periodicity.
In particular, the images produced according to its Fractal Forgeries paradigm always come with an x=y axis of symmetry.
What is the mathematical or numerical reason for that?
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Some books
The Science of Fractal Images
Authors: Michael F. Barnsley, Robert L. Devaney, Benoit B. Mandelbrot, Heinz-Otto Peitgen, Dietmar Saupe, Richard F. Voss
Editors: Heinz-Otto Peitgen, Dietmar Saupe
ISBN: 978-1-4612-8349-2 (Print) 978-1-4612-3784-6 (Online)
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I am wondering about how an aqueous suspension of superparamagnetic nanoparticles would behave if an externally applied uniform magnetic field were applied.  With no magnetic field, I assume the particles will move in a random motion as they collide with eachother and the water molecules--normal Brownian motion.
But what if the particles were inside a solenoid type of apparatus?  For example, the suspension was inside a glass capillary tube with a current carrying wire wrapped lengthwise around it.  
My question is, the instant you apply current and establish that magnetic field, how will the motion of the SP nanoparticles change?  
Without the magnetic field, each particle has 6 degrees of freedom (translational motion about x, y, z axes and rotational motion also about x, y, z).  If the x axis be taken as passing through the center of the horizontal capillary tube, then which of the 6 types of motion will be affected once the solenoid is activated?  
My thought is that translational motion will not change.  But the particle will be restricted to only rotating about the x axis (aligning itself with the magnetic field) and no longer rotate in the y and z.  Is that right?
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Dear Dr.: Lawler:
This is an interesting question, with several very interesting sub-questions. But there are a great number of concepts involved at each part, as mentioned. It is possible that an approach more constructive be based on a specific parts exploration. Then, at nanoparticles superparamagnetics, in addition to the superparamagnetism concepts, nanoparticles can be interacting ( high density of nanoparticle) or non-interacting, also can be single domain or non-single domains. At any combination, concept of critical radii of nanoparticle, total magnetic moment of nanoparticle and Exchange integral are realistic parameters.
In this way, each part of the major question is below reproduced and in the sequence each part of the answer is approached, as follow:
“I am wondering about how an aqueous suspension of superparamagnetic nanoparticles would behave if an externally applied uniform magnetic field were applied. With no magnetic field, I assume the particles will move in a random motion as they collide with each other and the water molecules--normal Brownian motion.”
Typically, fluids contain a very low nanoparticles concentration, this feature make impossible mechanical interaction between nanoparticles. Depending on the temperature and fluid medium density and viscosity, the phenomenon called Brownian motion can occurs with major or minor intensity, in fact another factor can be affect the Brownian motion as nanoparticle surface wettability and capability of the fluid of interact with surface from superficial charge-density of nanoparticle, consider see:
“But what if the particles were inside a solenoid type of apparatus? For example, the suspension was inside a glass capillary tube with a current carrying wire wrapped lengthwise around it. My question is, the instant you apply current and establish that magnetic field, how will the motion of the SP nanoparticles change? ”
It is necessary a clear vision of Magnetic behavior of matter and contribution of size effects or finite size effects on the magnetic-behaviour of the matter, consider see:
According to the Neel model there is a critical size of nanoparticles for that magnetic single domain state can be reached via Exchange interaction. In this sense, the superparamagnetic state can be further characterized as having a contribution of exchange interaction tending to null, but not null, by comparison with contribution of thermal energy.
A possible interpretation these characteristics phenomena is that a magnetic moment liquid ascribed to lattice atoms can be operational but its magnitude change (stable magnetic order is loosen) in the time domain due thermal effects or thermal fluctuation.
Seems that there are several models to the comprehension of the behavior of collection of nanoparticle based on a small set of assumption, someone complex intrinsically. The simplest model involves a collection of monodisperse of nanoparticles sizes and single domain nanoparticles.
In a broad sense, superparamagnetics nanoparticles will move in the fluid as a function of magnetization induced by magnetic field of solenoid. The movement of collection of particles depending on the direction of applied field, in fact at opposite direction is expected.
“Without the magnetic field, each particle has 6 degrees of freedom (translational motion about x, y, z axes and rotational motion also about x, y, z). If the x axis be taken as passing through the center of the horizontal capillary tube, then which of the 6 types of motion will be affected once the solenoid is activated?”
Well, I expect that understood the question. In fact, neither all nanoparticle exhibits spherical symmetry, typically oblate or more symmetric nanoparticle exist. Supposing that above discussed be satisfied, finite size effect, one domain (single domain) or two or more domains can be developed in a spherical nanoparticle. The magnetic moment of all atom belong to this domain will give a total magnetic moment with more or less contribution of exchange integral. After this, there is a vector magnetization that turn restricts the idea of several degrees of freedom. In this sense, the direction parallel and anti-parallel to the magnetization vector are now most relevant at nanoparticle since vector magnetic field stemming of solenoid is aligned to vector magnetization stemming of nanoparticles. Again, here, naturally, there is not magnetic interaction between nanoparticles.
“My thought is that translational motion will not change. But the particle will be restricted to only rotating about the x axis (aligning itself with the magnetic field) and no longer rotate in the y and z. Is that right?”
Is complicated to comment the non-existence of movement at perpendicular axes to the magnetization axis, but seems that is non-probable.
The paper of C. Stoner and E. P. Wohlfarth, as well as its models are basic to start an understanding the major question, consider see:
C. Stoner and E. P. Wohlfarth Trans. Magn. 27, 1991(reprinted)
More recently, consider see:
Also:
Best regards
Marcos Nobre
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This is probably a map algebra problem. I have a 2D map with values ranging 0.0 to 1.0 spread all over it. The algorithm that produces them is an application of the fractional Brownian motion. The map measures 101x101 pixels or cells.
My problem: I want to find in the map the regions (or islands) which values exceed a given threshold, e.g. 0.3 (we can call them the hotspots). I then want to calculate the number of pixels or cells that fall within the boundaries of that island. Given that there might be more than one island, I could end up with:
  1. Situation 1: 1 island with, say, 1000 pixels or cells;
  2. Situation 2: 2 islands with 500 pixels or cells each;
  3. Additional combinations.
Since I must be able to distinguish between the various situations, I was thinking of somehow weighing the total number of cells with respect to the number of islands. How could I do this, other than considering the average number of cells (which I see as a trivial solution)?
Please take a look at the picture for a better explanation of what I mean by islands or regions.
I would appreciate it if you could give me some direction, along with some relevant references. Thank you!
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Hi,
I would clip the raster to the layer of the islands, reclassify the raster with one classes (above 0.3 and the rest as nodata) and then do a zonal statistics for the island features with the reclassified raster as input value. Apart from the various statistics, the "zonal statistics as table" tool also produces the area of the raster inside the feature.
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I have a series of 2D maps with values ranging 0.0 to 1.0 spread all over. The algorithm that produces them is an application of the fractional Brownian motion. Each map measures 101x101pixels or cells.
The algorithm producing these maps uses a discretized Inverse Fast Fourier Transform (FFT) in the spectral domain. The maps have a varying mean (0.0 to 1.0) but share a fixed variance which is σ2 = 1. 
My question: it is said (check the attached link) that applying Moran's I to determine the clustering of a geographic dataset is sensitive to the dataset distribution, especially if the distribution is skewed. Since my algorithm produces maps which distribution is not consistent across all maps, what could be a robust algorithm for determining the clustering of my maps?
The aim is to find a method in which no influence is played by the shape of the distribution on the p-value of the clustering coefficient. 
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"My distribution is sometimes skewed, but not always...."
This is a nice property, which means that ht-index can capture the change or dynamics of the distribution; see the following figure, in which the shape of the trees is changing, implying that the distribution of all their branches is changing.
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I am interested to know whether the forces that cause brownian motion can help keep larger particle suspended in a fluid even though they are too large to show the movement.
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In general the Brownian motion is but sort of oscillations about the equillibrium point, or a steady path, so upon applying time averaging, this effect should zero out. However there are two things that  come into play, so the entire picture changes. Using the term "Brownian motion" you mean random movements of particles w/o referring to any equillibrium or steady path, as these are unknown to you. Secondary blood, if not all body fluids, is everything but a newtonian fluid. It has a memory. So such a fluid remembers (just to ilustrate this) that this particle was "going left", although it now "goes to the right".  I do not believe this would effect the action of gravity force per se, but in combination with "crowding out of heavier particles" under action of a cetrifugal forces in same body of the mixture, this could produce an apparent buoyant force. My insights may be very limited from this point on, because I have no experience with non-newtonian fluids. There is a group in the UK called FOAM, they deal in advanced comoutational fluid dynamic and may already have some software to lead you further on.  RGDS. Jerzy Klimkowski   
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Brownian motion can be see in starch grains that are approx 1micrometre in diameter.
What is the maximum size of particle before they can no longer exhibit Brownian Motion?
Platelets are 2 micrometres in diameter and are only marginally more dense than plasma. There are studies of the effects of Brownian Motion in flowing  fluids to mimic its effect in vivo, but I cannot find any reference to it being studied in plasma at rest. 
Has anybody seen any studies of Brownian Motion in Platelets at rest in non-flowing plasma? 
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I worked with platelets and was never able to see Brownian motion. They are flat disks in the resting state, and about 3 um in diameter. 
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Hi,
I am trying to write a code for fBm in Python. I am following the SpectralSynthesisFM2D pseudocode written by Dietmar Saupe in "The Science of Fractal Images", Springer-Verlag, 1988 (page 108). This pseudocode uses the spectral synthesis approach instead of the diamond-square algorithm.
I got stuck at lines 25-27, where the pseudocode calls something like A[][].imag, which has not been defined. I failed to "translate" this into a Python command.
Could anyone please help? Thanks!
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Dear Francesco,
As the the entries in the array A are complex numbers, I assume A[][].imag = 0 means set the imaginary part of the number to zero.
Steve
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I am trying to calculate the Hurst-Exponent for time-series I created (stock price). I tried to use DFA, DMA und GHE and wrote everything in python.
To test if I implemented it correctly I generated a fractional Brownian motion with an algorithm from here http://arxiv.org/pdf/1308.0399v1.pdf (p28-29) with several Hurst-Exponents. I found a matlab code for the GHE here:
The problem I face is that the H-values for my different methods differ quite a bit. For example fBm(H=0.3): DMA:0.286, DFA:0.336, GHE:0.309 , whereas the matlab-code has a precision of about 1%.
My first question is: Is it normal that the values differ this much? Might there still be an error somewhere in my code? I usually get at least under 10%.
Second: The H-value seems to depend a lot on how I chose the scaling window. If I use a series with length=2^16 how big should my windows be?
For DFA I cut them into 2^4..2^13 parts. For DMA and GHE I tried a lot of things like 5,6...,20 or 10,20,..100 or 10^1...10^5.
Is there a proper way to assign the windows? How do I get the exact H-value?
Is there even an "exact" value?
I really appreciate any help.
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Flo,  The best way to check your results is to plot them. Use log-log coordinates and plot the outputs of DFA and other methods you are using. You should be able to spot possible problems with the code and also you should be able to verify the scaling range of your time-series. Please remember that once you get close to sample size and to the sample resolution (max scale and min scale respectively) you will encounter finite size effects which affect your scaling estimate. Different methods respond differently to these finite size effects. Furthermore, there is no 'ideal' method which would recover the 'true' scaling exponent - all estimates suffer from finite size effects. Choosing the range of scaling (window sizes) is a bit of an 'art'. Generally, you need to choose the largest possible range, but sill stay away from gross finite size effects. Please also check earlier discussion of related matters with scaling estimates: https://www.researchgate.net/post/How_accurate_we_can_estimate_the_Fractal_Dimension/1
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Im trying to plot the dynamic brownian motion variance for my movement dataset using:
plot(Timestamp(var), getMotionVariance(var), type='s')
I received this error:
error in evaluating the argument 'x' in selecting a method for function 'plot'
This error wasn't cropping up before but now it is. 
I have attached the file below. 
Also, I want to plot the variance against time. How may I do so?
My timestamp is in the format: 4/17/2015 12:00
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    i wrote to the author and he corrected me, the function is timestamps. 
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I wonder to know how accurate might be an estimate of fractal dimension for a specific fBm?
I've created a bunch of fractals with the same known value of H, inside a loop and tried to estimate their fractal dimension but it seems there are some variations around the estimated values in comparision to the original H (or dF) that I started with!
Is this normal? Is there any approach or method to get more accurate estimations?
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Moein, it is very rare that you have to get the answer using just one pass estimation. In principle, you can always make a rough estimate first and then choose the method which works best in that range of H. In real life, I always used at least two methods and compared the results, often using various parameter settings such as # of vanishing moments with wavelets or degree of detrending using DFA. Integration prior to calculating H is another choice you need to make depending on where your H is. There is really no simple answer to your question from my experience. Once you see your results converging, you are likely working in the right direction using the right method (settings). 
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Brownian motion of nanoparticles
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In the absolute rate theory, which may be applicable to Brownian motion due to its stochastic nature,    the reaction rate constant  K+ is given by K+=  exp(-DelG/RT),  where Del G  is the Gibbs free energy of the activated complex particle at the saddle point configuration. One can also write  K+ = Gama+ C+/ GamaR CR,  where  +  denotes activated complex quantities.  C  is density of the nano particle at the reactant state. Then the rate of reaction is given by
  Rate= (RT/Nh) C+=  (RT/Nh)  K+ GamaR / Gama+  CR.  
N Avogadro number , h  planck constant.
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Molecules of  usual gas move stochastically. This stochasticity is a result of interaction between gas molecules (collisions of molecules). Let us imagine that molecules of the gas interacts by means of some force field. In this case the character of stochasticity of molecular motion changes. Let us take into account, that the wave function is a method of description of any ideal fluid motion (See  “Spin and wave function as attributes of ideal fluid.” J. Math. Phys.40, 256 -278, (1999). Electronic version http://gasdyn-ipm.ipmnet.ru/~rylov/swfaif4.pdf ). Is it possible to choose such a force field, that the gas with such interaction between molecules be described by the Klein-Gordon (or Schroedinger) equation? In other words, is it possible a classical description of quantum particles?
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Dear Humam,
You are right. There is a connection between quantum phenomena and the classical ones. But I should like to stress, that the quantum phenomena can be explained from the viewpoint of classical dynamics. It is very important, because in this case there is no necessity to quantize all in the world. In particular, one does not need to consider quantum gravitation, which is considered by some theorists as the main problem of  the elementary particle theory.
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If Markov and Martingale are properties of Brownian. What is Wiener then? How Markov is different from Martingale.
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In most sources, the Brownian Motion and the Wienner Process are the same things. However, in some sources the Wiener process is the standard Brownian motion while a general Brownian Motion is of a form αW(t) + β.
A Brownian  Motion or Wienner process, is both a Markov process and a martingale. These two properties are very different. In fact, they have little in common. A random process X_t, adapted to a filtration F_t, is a martingale with respect to the filtration if conditional expectation of the increment E( X_t - X_s | F_s) =0 for all t>s (conditional increment equals 0).
The same process has Markov property if 
E( X_t  | F_s) = E( X_t | X_s) =0 for all t>s (future distribution is independent of past).
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Hello all, I am investigating the sedimentation behavior of colloidal particles at different temperatures and using different grain size distributions. Sedimentation kinetics are affected by the inter-particle, gravity, and Brownian forces. I need to experimentally measure an index that can describe the Brownian effects, or theoretically estimate a value that correlate Brownian forces to the others. Any suggestions.
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There are a variety of techniques that you could use to measure the Brownian diffusion effects, including particle tracking microrheology and dynamic light scattering.
Whilst gravity will always be acting on your particles, the Brownian diffusion in the horizontal plane will not be effected by this, and similarly if you take measurements for a dilute suspension, inter particle interactions could also be ignored. 
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In the attached paper from the Gauge Institute, the definition of differential in e-calculus is (see page 8):
F'(x)={f(x+e)-f(x)}/e (1)
where e is defined as an infinitesimal (i.e. it should be smaller than any number but greater than zero).
From this definition in (1) it should be clear that as e approaches zero, it is assumed that the function of f'(x) has the form of a slope (linear). But this assumption has problems in real data of many phenomena, i.e. when the observation scale goes smaller and smaller then it behaves not as a linear slope but as brownian motion. Other applications such as in earthquake data, stock market price data, etc. indicate that each data includes indeterminacy (I).
I just thought that perhaps we can extend the definition of differentiation to include indeterminacy (I), perhaps something like this:
F'(x)={f(x+e)+2I-f(x)}/e. (2)
The I parameter implies that the geometry of differential is not a slope anymore. The term 2I has been introduced to include unpredictability/indeterminacy of the brownian motion. And it can split into left and right differentiation. The left differential will carry one I, and the right differential will carry one I.
Another possible way is something like this:
F'(x)=(1+I).{f(x+e)-f(x)}/e (3)
Where I represents indeterminacy parameter, ranging from 0.0-0.5.
Other possible approaches may include Nelson's Internal Set Theory, Fuzzy Differential Calculus, or Nonsmooth Analysis.
My purpose is to find out how to include indeterminacy into differential operators like curl and div.
That is my idea so far, you can develop it further if you like. This idea is surely far from conclusive, it is intended to stimulate further thinking.
So do you have other ideas? Please kindly share here. Thanks
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Calculus ultimately relies on infinite precision, the differential being infinitessemal, i.e. the next number to zero. In many instances this causes no problems even if it is mathematical garbage. Some authors now state than their differential is a small number not an infinitessimal then procced using the normal methods of calculus. Where Nature disagrees then we end up with contradictions like the UV catastrophy. Since we do not know when Nature will not bowl us a googly we should always check that taking the differential to be arbtrary small actually works. This is seldom done so there is no literature on this. There is no a priori method of introducing indeterminacy to calculs but if indeterminacy exists in Nature, she will let us know if we ask the right questions. Planck set up his differential of action and increased the pecission of his calculations  he found that when da = h he got the correct spectrum but lost it again when da<h Thus he found the indetrminacy in his calculus. I have never seen any other method than try it and see.
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Start with a reflexion domain  being a polygon A1 A2 ...An, with n summits
A simple computation using formula line 7 page 57 shows that if d(An, An-1)-->0 then P (B5(0)=An)-P(B5(0)=An-1)-->0 as n-->infinity
and P((B5(t+s)€E/B5(0)=An))-P((B5(t+s)€E/B5(0) =An-1))-->0 as n--> infinity
Which allow to derive the distribution of the relected process in a bounded domain with smooth boundaries.
Thanks
Bernard Bellot
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Why don't you upload the article for easy visibility?
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I want to run Brownian Dynamics simulation and wonder which software package is more popular? 
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LAMMPS and GROMACS are popular simulation packages for molecular dynamics (MD) simulations. Both can be used to simulate Brownian Dynamics by using Langevin dynamics. See "fix langevin" in LAMMPS or "bd integrator" in GROMACS.
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How does it vary with concentration, temperature, size of atom? 
My question is related to diffusion process.
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There is a Gibbs energy barrier between two stable positions of a ion. To go from one stable position to another, the ion must overcome this barrier. This is possible because the ion is not frozen - it vibrates around its equilibrium position and each time it vibrates towards the barrier, there is a possibility of surpassing it. Let f0 be the frequency with which the ion tries to overcome the barrier by vibrating towards the barrier (the so-called attempt frequency). The jump frequency f is then given by
                              f = f0 * exp [ - G / kT ],
in which G is the Gibbs energy of migration from one stable position to another (height of the barrier), k is the Boltzmann's constant and T is temperature. The exponential term corresponds to the probability of surpassing the barrier at each try.
The form of the equation above shows clearly that the jump frequency increases with temperature. And this is reinforced by the fact that G usually decreases as the temperature increases.
The effect of ion size and concentration on the jump frequency is via G. Usually, the smaller and lighter the ion, the lower is the barrier, resulting in greater jump frequencies. The effect of concentration of defects on G, on the other hand, is less obvious. High concentration of defects can lead to structural distortions and/or defect interactions, for instance, that can increase or reduce G.
One way to investigate the effect of concentration on G, and consequently on f, is by computational modeling. I recommend the GULP program, by Julian Gale.
PS: Even for a given ion with a given concentration in a fixed temperature, there may be more than one possible migration routes, with different Gs (leading to different fs), one for each route. Again, this can be investigated by computer simulations, as in the paper attached.
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I need to run an atomistic molecular dynamics simulation of a system in which some neutral gold atoms are randomly distributed in water box. I need to see how the gold atoms behave in water with time. But for running the simulation I need correct polarizable forcefield for gold atoms in water. There are some papers in which forcefields of various types of gold surface are present, but not for single gold atoms. Can anybody provide me any clue about the polarizable forcefield of single gold atom in water?
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Wouldn't singular gold atoms react with the water to form some hydrated Au + or Au 2+ ions?
I guess if you do gold (nano) particles in water that potential for gold surfaces is already quite good.
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Looking for main QoS parameters (loss probability, queue length, mean delay and response time) for FBM input, Pareto input, FARIMA input and other known proccesses.
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I do not see any analytic papers on fractional ARIMA calculation. I agree with you that this is a gap. That is PhD work-to-be done. In my queueing paper, we conquered the M/M/r/K/K calculation. It may inspire your work.
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Although we can see the result from Brownian motion that small particles in the fluid actually have random movement, which means these fluctuations are unsymmetrical, I still don't know why in statistics we can say in small intervals of time these fluctuations would be unsymmetrical?
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I see. Thank you very much!
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When or where do we use both?
Thanks.
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Different statistical distribution base :-)
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Due to the non-conservative nature of radiation pressure force, it can be used for the cooling of atomic motion.
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There are, however, conservative force traps which also use laser beams - the dipole traps. A blue-detuned laser beam when focued on laser-cooled atoms can trap the atoms. This kind of trap is 'conservative' in the sense that the the flow of energy is both ways between the atoms and the laser beams. The optical force in such traps arises from the intensity gradient of the laser beam at the focus...Good Luck!
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can anybody explain to me about : 
1 - When the nanofluid is heated the nanoparticles experience stronger Brownian motion ?
2- Stronger Brownian motion leads to  increase the amount of aggregation ?
3- Aggregation causes thermal conductivity enhancement ?
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Dear Hamid,
I'd like to add some points about your question from a brief literature review point of view. A number of possible mechanisms have been proposed for the enhancement of effective thermal conductivity, which included Brownian motion effect, interfacial liquid layering, clustering and networking. We are facing 2 different ways: For nanofluids application under forced convective conditions, possible contributions to the complex behavior of the nanofluids may include the Brownian motion, particle rotation and its associated micro convection, particle migration and the resulting non-uniform property profile, and suppression or interruption of the boundary layer. The mechanisms associated with nanofluids under natural convective heat transfer conditions are expected to be quite different including particle-fluid slip and sedimentation of nanoparticles.
For more info about your no. 3 question, please look at our publication (http://dx.doi.org/10.1007/s10973-014-4048-0)
Good luck
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Random motion of gaseous molecules was one of the assumptions used to facilitate derivation of gas laws. Yet it is currently accepted as real displacements (vibrations in cases of solid and liquid) of molecules in space. Could someone explain on what basis this assumption became a real fact?
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In a celebrated paper published in 1905  by A.Einstein, the motion of pollen grains in water (i.e. Brownian motion) was calculated on the basis of molecular nature of water and random collisions of these molecules with the grains that results in a mean squared displacement proportional to time and diffusion constant, this paper historically proved the molecular nature of water and relation of their mean velocity with  temperature. On the other hand the definition of "temperature"  based on the motion (kinetic) of molecules and famous works conducted by Boltzmann and Maxwell had been shown that the assumption of atomic or molecular nature plus the random motion of them could obtain a consistent theory for definite description of  macroscopic thermodynamical parameters such as temperature, pressure, heat conduction and internal energies of systems compatible with thermodynamic laws.Moreover this assumptive motion has been observed directly by electron microscopy and STM etc.