L. Wolfenstein’s research while affiliated with Carnegie Mellon University and other places

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Publications (163)


Review of particle physics: Particle data group
  • Article

January 2016

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48 Reads

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227 Citations

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K. Agashe

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G. Aielli

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[...]

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P.A. Zyla

Figure 1.2: Band-power estimates from the Planck, WMAP, ACT, and SPT experiments. Note that the widths of the-bands vary between experiments and have not been plotted. This figure represents only a selection of the most recent available experimental results, and some points with large error bars have been omitted. At the higher multipoles these band-powers come from subtraction of particular foreground models, while proper analysis requires simultaneous fitting of CMB and foregrounds over multiple frequencies. The multipole axis here is linear, so the Sachs-Wolfe plateau is hard to see. However, the acoustic peaks and damping region are very clearly observed, with no need for a theoretical curve to guide the eye; the curve plotted is a best-fit model from Planck plus other CMB data. 
Figure 1.1: Power spectrum of B-mode polarization, including results from the BICEP2 [78], POLARBEAR [79], and SPT (derived from a lensing correlation analysis) [60] experiments. Note that several experiments have previous reported upper limits, which are all off the top of this plot. A logarithmic x-axis is adopted here and the y-axis has been divided by a factor of √ in order to show all three theoretically expected contributions: the low-reionization bump, ∼ 100 primordial tensor peak, and high-lensing signature. The dotted line is for a tensor (gravitational wave) fraction r = 0.2, simply to guide the eye, with all other cosmological parameters set at the best Planck-derived values, for which model the expected lensing B-modes have also been shown with a dashed line. 
Figure 1.4: Power spectrum of E-mode polarization from several different experiments, plotted along with a theoretical model that fits Planck plus other CMB data. Note that the widths of the bands have been suppressed for clarity, but that in some cases they are almost as wide as the features in the power spectrum. 
Figure 1.3: Cross power spectrum of the temperature anisotropies and Emode polarization signal from WMAP, together with estimates from BICEP, BOOMERANG, CBI, DASI, and QUAD, several of which extend to higher. The curve is the prediction from the best fit to the temperature band-powers (with a prior from ≤ 23 polarization) and is not a fit to these data. Note that the y-axis here is not multiplied by the additional , which helps to show both the large and small angular scale features. 
Review of Particle Physics
  • Article
  • Full-text available

January 2014

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856 Reads

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8,846 Citations

Chinese Physics C

The Review summarizes much of particle physics and cosmology. Using data from previous editions, plus 3,283 new measurements from 899 papers, we list, evaluate, and average measured properties of gauge bosons and the recently discovered Higgs boson, leptons, quarks, mesons, and baryons. We summarize searches for hypothetical particles such as heavy neutrinos, supersymmetric and technicolor particles, axions, dark photons, etc. All the particle properties and search limits are listed in Summary Tables. We also give numerous tables, figures, formulae, and reviews of topics such as Supersymmetry, Extra Dimensions, Particle Detectors, Probability, and Statistics. Among the 112 reviews are many that are new or heavily revised including those on: Dark Energy, Higgs Boson Physics, Electroweak Model, Neutrino Cross Section Measurements, Monte Carlo Neutrino Generators, Top Quark, Dark Matter, Dynamical Electroweak Symmetry Breaking, Accelerator Physics of Colliders, High-Energy Collider Parameters, Big Bang Nucleosynthesis, Astrophysical Constants and Cosmological Parameters.

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Transmission of neutrinos through matter

April 2012

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22 Reads

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4 Citations

Pramana

Neutrinos travel through matter with negligible absorption except in very extreme situations. However, the index of refraction of neutrinos can play an important role in the oscillation of one type of neutrino to another when passing through matter.


Review of Particle Physics

July 2010

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3,466 Reads

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5,524 Citations

This biennial Review summarizes much of particle physics. Using data from previous editions, plus 2158 new measurements from 551 papers, we list, evaluate, and average measured properties of gauge bosons, leptons, quarks, mesons, and baryons. We also summarize searches for hypothetical particles such as Higgs bosons, heavy neutrinos, and supersymmetric particles. All the particle properties and search limits are listed in Summary Tables. We also give numerous tables, figures, formulae, and reviews of topics such as the Standard Model, particle detectors, probability, and statistics. Among the 108 reviews are many that are new or heavily revised including those on neutrino mass, mixing, and oscillations, QCD, top quark, CKM quark-mixing matrix, V-ud & V-us, V-cb & V-ub, fragmentation functions, particle detectors for accelerator and non-accelerator physics, magnetic monopoles, cosmological parameters, and big bang cosmology. A booklet is available containing the Summary Tables and abbreviated versions of some of the other sections of this full Review. All tables, listings, and reviews (and errata) are also available on the Particle Data Group website: http://pdg.1b1.gov.


Review of Particle Physics

January 2010

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788 Reads

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3,055 Citations

The European Physical Journal C

This biennial Review summarizes much of particle physics. Using data from previous editions, plus 2158 new measurements from 551 papers, we list, evaluate, and average measured properties of gauge bosons, leptons, quarks, mesons, and baryons. We also summarize searches for hypothetical particles such as Higgs bosons, heavy neutrinos, and supersymmetric particles. All the particle properties and search limits are listed in Summary Tables. We also give numerous tables, figures, formulae, and reviews of topics such as the Standard Model, particle detectors, probability, and statistics. Among the 108 reviews are many that are new or heavily revised including those on neutrino mass, mixing, and oscillations, QCD, top quark, CKM quark-mixing matrix, V-ud & V-us, V-cb & V-ub, fragmentation functions, particle detectors for accelerator and non-accelerator physics, magnetic monopoles, cosmological parameters, and big bang cosmology.


Particle physics booklet

January 2010

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4,783 Reads

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30 Citations

This biennial Review summarizes much of particle physics. Using data from previous editions, plus 2158 new measurements from 551 papers, we list, evaluate, and average measured properties of gauge bosons, leptons, quarks, mesons, and baryons. We also summarize searches for hypothetical particles such as Higgs bosons, heavy neutrinos, and supersymmetric particles. All the particle properties and search limits are listed in Summary Tables. We also give numerous tables, figures, formulae, and reviews of topics such as the Standard Model, particle detectors, probability, and statistics. Among the 108 reviews are many that are new or heavily revised including those on neutrino mass, mixing, and oscillations, QCD, top quark, CKM quark-mixing matrix, Vud & Vus , Vcb & Vub, fragmentation functions, particle detectors for accelerator and non-accelerator physics, magnetic monopoles, cosmological parameters, and big bang cosmology. A booklet is available containing the Summary Tables and abbreviated versions of some of the other sections of this full Review. All tables, listings, and reviews (and errata) are also available on the Particle Data Group website: pdg.lbl.gov.


Review of particle physics

January 2010

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55 Reads

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261 Citations

This biennial Review summarizes much of particle physics. Using data from previous editions, plus 2158 new measurements from 551 papers, we list, evaluate, and average measured properties of gauge bosons, leptons, quarks, mesons, and baryons. We also summarize searches for hypothetical particles such as Higgs bosons, heavy neutrinos, and supersymmetric particles. All the particle properties and search limits are listed in Summary Tables. We also give numerous tables, figures, formulae, and reviews of topics such as the Standard Model, particle detectors, probability, and statistics. Among the 108 reviews are many that are new or heavily revised including those on neutrino mass, mixing, and oscillations, QCD, top quark, CKM quark-mixing matrix, Vud & Vus, Vcb & Vub, fragmentation functions, particle detectors for accelerator and non-accelerator physics, magnetic monopoles, cosmological parameters, and big bang cosmology.


DUSEL theory white paper

November 2008

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592 Reads

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30 Citations

The NSF has chosen the site for the Deep Underground Science and Engineering Laboratory (DUSEL) to be in Lead, South Dakota. In fact, the state of South Dakota has already stepped up to the plate and contributed its own funding for the proposed lab, see http://www.sanfordlaboratoryathomestake.org/index.html. The final decision by NSF for funding the Initial Suite of Experiments for DUSEL will be made early in 2009. At that time the NSF Science Board must make a decision. Of order 200 experimentalists have already expressed an interest in performing experiments at DUSEL. In order to assess the interest of the theoretical community, the Center for Cosmology and Astro-Particle Physics (CCAPP) at The Ohio State University (OSU) organized a 3-day DUSEL Theory Workshop in Columbus, Ohio from April 4 - 6, 2008. The workshop focused on the scientific case for six proposed experiments for DUSEL: long baseline neutrino oscillations, proton decay, dark matter, astrophysical neutrinos, neutrinoless double beta decay and N-Nbar oscillations. The outcome of this workshop is the DUSEL Theory White paper addressing the scientific case at a level which may be useful in the decision making process for policy makers at the NSF and in the U.S. Congress. In order to assess the physics interest in the DUSEL project we have posted the DUSEL Theory White paper on the following CCAPP link http://ccapp.osu.edu/whitepaper.html . Please read the white paper and, if you are interested, use the link to show your support by co-signing the white paper.


Review of Particle Physics

September 2008

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214 Reads

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5,580 Citations

Physics Letters B

This biennial Review summarizes much of particle physics. Using data from previous editions, plus 2658 new measurements from 644 papers, we list, evaluate, and average measured properties of gauge bosons, leptons, quarks, mesons, and baryons. We summarize searches for hypothetical particles such as Higgs bosons, heavy neutrinos, and supersymmetric particles. All the particle properties and search limits are listed in Summary Tables. We also give numerous tables, figures, formulae, and reviews of topics such as the Standard Model, particle detectors, probability, and statistics. Among the 112 reviews are many that are new or heavily revised including those on Heavy-Quark and Soft-Collinear Effective Theory, Neutrino Cross Section Measurements, Monte Carlo Event Generators, Lattice QCD, Heavy Quarkonium Spectroscopy, Top Quark, Dark Matter, V-cb & V-ub, Quantum Chromodynamics, High-Energy Collider Parameters, Astrophysical Constants, Cosmological Parameters, and Dark Matter. A booklet is available containing the Summary Tables and abbreviated versions of some of the other sections of this full Review. All tables, listings, and reviews (and errata) are also available on the Particle Data Group website: http://pdg.lbl.gov.


Consequences of Approximate S3S_3 Symmetry of the Neutrino Mass Matrix

October 2007

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34 Reads

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56 Citations

Physical Review D

Assuming that the neutrino mass matrix is dominated by a term with the permutation symmetry S3S_{\scriptscriptstyle 3} it is possible to explain neutrino data only if the masses are quasi-degenerate. A sub-dominant term with an approximate μτ\mu -\tau symmetry leads to an approximate tri-bimaximal form. Experimental consequences are discussed.


Citations (54)


... En este sector no se presenta un término de masa en si, se presenta un matriz de masa M, una para los quark tipo u, una para los quarks tipo d y una los leptones. Las masas físicas (aquellas que se miden experimentalmente) se interpretan como los eigenva-lores de la matriz de masa M. En el contexto del ME, la estructura de la matriz de masa para los quarks es completamente desconocida, elúnico indicio que se tiene es la matriz Cabibbo Kobayashi Maskawa V CK M (Olive et al. (2014), Branco et al. (1999)) que cuantifica los procesos débiles del W + y los quarks, el cuadrado de cada uno de los nueve elementos de esta matriz representa la probabilidad para que un quark tipo u se convierta en un quark tipo d a través de un W + . Del experimento, las masas de los quarks presentan el siguiente patrón m u < m c < m t ; m d < m s < m b ; conocido como jerarquía (Olive et al. (2014), Branco et al. (1999)). ...

Reference:

Análisis de texturas de 4 ceros
Review of particle physics: Particle data group
  • Citing Article
  • January 2016

... This corresponds to the time of the QCD phase transition, where the strongly interacting constituents, i.e. the quarks and gluons, are converted into hadrons. For a brief but concise description, see section 22.3 of [41]. In the QGP of the early universe, particles interacting via the strong and electro-weak force are part of the system, while an accelerator-made QGP only contains strongly interacting particles. ...

Review of Particle Physics

Chinese Physics C

... Since this parameter has units of length, it is natural to simulate real motion by considering Robin BC with time-dependent parameters, as explored in Ref. [73]. 9 The name "photon" was not coined by Einstein, but by the chemist Gilbert N. Lewis in 1926. In a letter to Nature [85], Lewis wrote: "I therefore take the liberty of proposing for this hypothetical new atom, which is not light but plays an essential part in every process of radiation, the name photon". ...

Review of Particle Physics

The European Physical Journal C

... can not be a constant of motion [16], this statement is not necessarily a request, [17], therefore, it is not so direct to make the identification and transition of the classical problem to the quantum problem. However, from the mathematical point of view, the quantum theory must be able to address these types of problems. ...

Particle physics booklet

... To create a pion, the CR proton must have a total energy (rest mass plus kinetic energy) greater than approximately 1.22 GeV (Kelner et al., 2006). The pions decay quickly -charged pions have lifetimes of 2.6 × 10 −8 s and neutral pions have lifetimes of 8.5 × 10 −17 s (Zyla et al., 2020). Depending on the charge of pion, the decay produces rays, muons ( ), or neutrinos ( ). ...

Review of particle physics
  • Citing Article
  • January 2010

... C 0 1;2;3 are found from C 1;2;3 by exchanging λ L ↔ λ R . The SM prediction is currently unclear, as a naive calculation gives a result four or five orders of magnitude too small, while other estimates (albeit not from first principles) suggest the SM alone could give a result x SM ∼ 0.1% [131][132][133][134][135][136][137], where ...

D00 mixing
  • Citing Article
  • December 1985

Physics Letters B

... The exact mechanism of this violation during baryogenesis remains a mystery. However, as of yet, no theoretical consensus has been reached regarding this, and there is no experimental evidence of an imbalance in the creation rates of matter and antimatter (Kolb and Turner, 1988;Wolfenstein, 1989;Bigi, 1997;Trodden, 1998;Utpal, 2007;Sozzi, 2008;Canetti et al., 2012). ...

CP violation
  • Citing Article
  • July 1995

... Let's set the scene. Assuming the unitarity of the CKM matrix is preserved (valid in a large class of BSM models), and that the most significant BSM effects occur in observables that vanish at tree level in the SM [11][12][13][14] 1 , the possible effects of heavy particles in each neutral meson system can be accounted for by two real parameters, ...

CP violation in the decays B0-->ΨKS and B0-->π+π-: A probe for new physics
  • Citing Article
  • February 1993

Physical Review D