Allan Widom’s research while affiliated with Northeastern University and other places

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Publications (45)


Figure 2: Theoretical vs measured total activity of Cu RI (in Bq) as a function of time.
Figure 3: The spectrum of Teflon target number 1 after irradiation. The annihilation peak (511 keV) is very visible
Original Research Article Generation of radio nuclides
  • Article
  • Full-text available

June 2021

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200 Reads

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Allan Widom

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Non-chemical signatures of biological materials: Radio signals from Covid19?

August 2020

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308 Reads

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5 Citations

Electromagnetic Biology and Medicine

All therapeutic methods dealing with coronavirus (past and present) are based on chemicals. We test for it (positive or negative) chemically and hope to cure it with a future vaccine (some complicated chemical preparation). If and when the virus mutates, another set of chemical protocols for its testing and a hunt for new chemicals as a vaccine shall begin again and again. But the history of modern (western) medicine tells us that our biotechnology is not so limited. Copious scientific evidence for sonic and low energy electromagnetic signals produced by all biological elements (DNA, cells, bacteria, parasites, virus) exists; in turn, the biological elements are affected by these non-chemical signals as well. A careful analysis and a catalogue of the spectrum of these non-chemical signals are proposed here as a unique biophysical signature.






Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy

May 2016

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430 Reads

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159 Citations

Physical Review Letters

We measure the energy emitted by extensive air showers in the form of radio emission in the frequency range from 30 to 80 MHz. Exploiting the accurate energy scale of the Pierre Auger Observatory, we obtain a radiation energy of 15.8 \pm 0.7 (stat) \pm 6.7 (sys) MeV for cosmic rays with an energy of 1 EeV arriving perpendicularly to a geomagnetic field of 0.24 G, scaling quadratically with the cosmic-ray energy. A comparison with predictions from state-of-the-art first-principle calculations shows agreement with our measurement. The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers. Comparison with our result thus allows the direct calibration of any cosmic-ray radio detector against the well-established energy scale of the Pierre Auger Observatory.


Figure 2
Polarization map of a single event. The axis coordinates are in the shower plane where the x axis corresponds to the direction of the Lorentz force (v→×B→) and the y axis perpendicular to that and to the shower axis [v→×(v→×B→)]. The SD shower core is at the coordinate origin. The measured polarizations are shown as the black arrows. The gray arrows are the model expectations, and the red and blue arrows are the geomagnetic and the charge-excess components, respectively. The definition of β is described in the text. The air-shower properties of this event are energy of 0.9 EeV and arriving from a zenith angle of 36° and from 27° south of west. For the emission model of Eq. (2), the optimal value of the relative charge-excess strength is a=0.18.
Figure 4
Skymap of the 126 selected events. Green solid circles denote air showers with at least five stations with signal and open circles denote air showers with less than five stations with signal. The red star denotes the direction of the magnetic-field axis at AERA. All measured events are at least 20° away from the magnetic-field axis. Therefore, the geomagnetic emission gives the dominant contribution to the radiation energy for all events.
Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory

August 2015

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441 Reads

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134 Citations

Physical Review D

The Auger Engineering Radio Array (AERA) is part of the Pierre Auger Observatory and is used to detect the radio emission of cosmic-ray air showers. These observations are compared to the data of the surface detector stations of the Observatory, which provide well-calibrated information on the cosmic-ray energies and arrival directions. The response of the radio stations in the 30 to 80 MHz regime has been thoroughly calibrated to enable the reconstruction of the incoming electric field. For the latter, the energy density is determined from the radio pulses at each observer position and is interpolated using a two dimensional function that takes into account signal asymmetries due to interference between the geomagnetic and charge excess emission components. The spatial integral over the signal distribution gives a direct measurement of the energy transferred from the primary cosmic ray into radio emission in the AERA frequency range. We measure 15.8 MeV of radiation energy for a 1 EeV air shower arriving perpendicularly to the geomagnetic field. This radiation energy -- corrected for geometrical effects -- is used as a cosmic-ray energy estimator. Performing an absolute energy calibration against the surface-detector information, we observe that this radio-energy estimator scales quadratically with the cosmic-ray energy as expected for coherent emission. We find an energy resolution of the radio reconstruction of 22% for the data set and 17% for a high-quality subset containing only events with at least five radio stations with signal.



Citations (32)


... The role played in structured interfacial water CD/EZ by sonic signals (phonons) and non-ionizing EM radiation (photons) 2 emitted and absorbed by biological systems, which do not cause thermal or heating effects but do cause non-thermal biological effects on electron and proton transfer reactions, en-zymes, DNA and fluxes in the ion channels of excitable membranes, is currently ignored or neglected. Likely, among the biophysical modalities involved in the pathogenicity of SARS-CoV-2 (severe acute respiratory syndrome coronavirus 2) and in addition to the classical electrostatic modality, other modalities based sonic signaling and on ULF-EMF signaling [17] should be taken into account. The present work points at introducing the possible ULF-EMF interactions. ...

Reference:

A Biophysical Approach to SARS-CoV-2 Pathogenicity Received: 11/11/2021 Accepted: 16/11/2021 Published: 27/12/2021
Non-chemical signatures of biological materials: Radio signals from Covid19?

Electromagnetic Biology and Medicine

... This construction inherently necessitates the use of relativistic Dirac fermions. The need for Dirac fermions in chemistry and condensed matter has previously been reported in Ref. [27]. The requirement of relativistic 4-component Dirac spinors in the description of condensed matter systems is relevant, for example, in heavy nucleon compounds, where Z 1. ...

The Dirac Equation in Low Energy Condensed Matter Physics

... In the field of astroparticle physics, a fundamental quantity used by high-level analyses is the energy fluence, i.e., the energy per unit area deposited on the ground in the form of radio waves [2]. The energy fluence measured in the presence of noise at the antenna position is given by: ...

Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy

Physical Review Letters

... This method turns out to be biased at low SNR values and underestimates the uncertainties (see figure 1). To avoid the introduction of a large bias, a minimum required SNR value is typically introduced to use data from a given antenna (in many works, SNR values of at least 10, when referring to the peak electric field amplitude squared divided by the noise variance, are required [5]). ...

Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory

Physical Review D

... More recently, Gerald Pollack and his team in Washington University came up with an idea to build a water battery model. [5] Allan Widom et al. also came up with a theory of waterbattery system [6]. ...

Theory of the Water Battery

... [40][41][42]. We also show the current upper limits on the cosmogenic neutrino flux at very high-energies from Auger [43], IceCube [44] and ANITA [45]. We also show sensitivity projections from GRAND200k (10 yr) and IceCube-Gen2 radio (10 yr) [46,47]. ...

Improved limit to the diffuse flux of ultrahigh energy neutrinos from the Pierre Auger Observatory

Physical Review D

... Quite independently, there have been studies of nuclear transmutations triggered by smart materials (such as, piezoelectrics, ferro-magnetics) under severe stress [3][4][5][6][7][8] , and of pyro-electrics undergoing changes in temperature [9,10] . The underlying electro-strong (ES) theory describing phenomena for materials under stress is based on the well known giant dipole resonances (GDR) that is briefly described in Sec. ...

Induction of Nuclear Reactions Through Piezoelectrics and Other Means

... On the other hand, there are also quantum mechanical-free electron motion along the effective perimeter of the material. The quantum mechanical electromagnetic (EM) transition frequencies are given by (Swain et al. 2013; ν n;qm ðLÞ ¼ ð π� h mL 2 Þð2n þ 1Þ; n ¼ 0; 1; 2; 3; . . . :; ν 1 : ν 2 : ν 3 . . . ...

Wireless Electromagnetic Communication Systems Between Bacteria in Communities

... The energy region where GCRs give room to extragalactic cosmic rays (EGCRs), somewhere between the second knee and the ankle, is particularly important to draw a complete description of the origin of UHECRs. In the region immediately below and around the ankle, a dominance of Galactic protons and medium-mass nuclei can be excluded based on the measured low level of anisotropy in the distribution of arrival directions [18,19]. On the other hand, a dominance of heavier nuclei, which would comply with the allowed limits, is disfavoured by the interpretation of X max measurements as mentioned above. ...

Constraints on the Origin of Cosmic Rays above 10^18 eV from Large-scale Anisotropy Searches in Data of the Pierre Auger Observatory

The Astrophysical Journal Letters

... To exclude events where the recorded profile may be distorted due to clouds over the Observatory, only events from known cloud-free periods are accepted. Events where no information on the cloud coverage is available from either the Lidar system installed at the FD site Coihueco (BenZvi et al. 2007) or infrared data from the GOES-12 satellite (Abreu et al. 2013) are excluded. ...

Identifying Clouds over the Pierre Auger Observatory using Infrared Satellite Data
  • Citing Article
  • December 2013

Astroparticle Physics