Results 251 to 260 of about 5,576,092 (280)

China's top 10 breakthroughs in science and technology in 2024. [PDF]

Natl Sci Rev
Zhu H.
europepmc   +1 more source

The waning of the WIMP: endgame? [PDF]

Eur Phys J C Part Fields
Arcadi G, Cabo-Almeida D, Dutra M, Ghosh P, Lindner M, Mambrini Y, Neto JP, Pierre M, Profumo S, Queiroz FS.   +9 more
europepmc   +1 more source

PRyMordial: the first three minutes, within and beyond the standard model. [PDF]

Eur Phys J C Part Fields
Burns AK, Tait TMP, Valli M.
europepmc   +1 more source

Parity and time-reversal violating nuclear forces with explicit Δ -excitations. [PDF]

Eur Phys J A Hadron Nucl
Gandor L, Krebs H, Epelbaum E.
europepmc   +1 more source

Silicon Drift Detectors for the Measurement and Reconstruction of Beta Spectra. [PDF]

Sensors (Basel)
Nava A, Bernardini L, Biassoni M, Bradanini T, Carminati M, De Gregorio G, Fiorini C, Gagliardi G, Lechner P, Mancino R, Brofferio C.   +10 more
europepmc   +1 more source

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The Physics of Neutrino Interactions

, 2020
This advanced text discusses the fundamental concepts of neutrinos, their properties and interactions with matter, presenting a theoretical framework for describing relativistic particles.
M. Athar, S. Singh, M. Sajjad, Athar S. K. Singh, ©. M. S. Athar   +4 more
semanticscholar   +1 more source

Interactions of neutrinos with matter

Progress in Particle and Nuclear Physics, 2017
Abstract Neutrinos are elementary particles electrically neutral which belong to the family of leptons. As a consequence and in first approximation they only undergo weak processes. This gives them very special properties. They are ideal tools to study precisely the weak interactions, but there is a price to pay: neutrinos are characterized by ...
openaire   +4 more sources

Interaction of neutrinos with matter

Il Nuovo Cimento A, 1974
An equation of motion for neutrinos in matter is presented. Solutions are obtained for neutrino motion in uniformly rotating current distributions. Implications for stellar neutrino emission are considered.
L. F. Landovitz, W. M. Schreiber
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Weak Interactions and Neutrinos

2011
The Sun will shine for 5 billion years (after the past first 5 billion years) because of the weak interaction. The study of the weak interaction is closely connected to that of the neutral lepton called neutrino. We shall focus on: the weak interaction universality; the Feynman diagrams of charged and neutral current interactions of hadrons and leptons;
Giorgio Giacomelli, Sylvie Braibant, Maurizio Spurio   +2 more
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Neutrino-nucleus interactions

The European Physical Journal A, 2007
Inclusive electron scattering cross-sections in the quasielastic and resonance regions for few GeV electrons are well represented in terms of scaling functions and scaling variables, the so-called superscaling analysis (SuSA). The concepts of scaling of the first and second kinds and superscaling are discussed, as are several mechanisms which are known
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