Results 111 to 120 of about 85,993 (252)
Nuclear Physics BIn this study, the charged particle multiplicity distribution produced in anti-neutrino and neutrino-nuclear emulsion interactions is studied in terms of negative binomial distribution in varying invariant mass of the hadronic system intervals for the ...
Çağın Kamışcıoğlu
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Ab initio calculation of the electromagnetic and neutral-weak response functions of 4He and 12C
EPJ Web of Conferences, 2016 Precise measurement of neutrino oscillations, and hence the determination of their masses demands a quantitative understanding of neutrino-nucleus interactions. To this aim, two-body meson-exchange currents have to be accounted for along within realistic
Lovato A. +6 more
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Advanced Functional Materials, Volume 35, Issue 2, January 9, 2025.Many modern detector systems require structured scintillators in combination with photo‐detectors. This requirement can be fulfilled by 3D printing plastic scintillators which becomes more and more relevant. However, the resolution and surface quality of 1‐photon‐based 3D printing techniques are not sufficient for many applications.
Jannis Weinacker +8 more
wiley +1 more source
A Brief, Biased View of Neutron Star Cooling
Astronomische Nachrichten, Volume 346, Issue 1, January 2025.ABSTRACT This is a concise and non‐technical review of topics related to neutron star (NS) cooling, for both young NSs and NSs in low‐mass x‐ray binaries. Neutrino emission from the NS core drives cooling rates, via different processes including Urca processes and pair breaking and formation at the neutron superfluid critical temperature.
Craig Heinke
wiley +1 more source
, 2011 The advent of very high intensity neutrino beams for the study of neutrino oscillations has also made possible a new generation of experiments which will study neutrino interactions on different nuclei with unprecedented precision. The use of the neutrino as a probe of nucleon structure provides unique information not available with other probes.
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Advances in High Energy Physics, Volume 2025, Issue 1, 2025.We obtain the off‐shell nilpotent Becchi–Rouet–Stora–Tyutin (BRST) and anti‐BRST symmetry transformations (corresponding to the infinitesimal classical gauge symmetry transformations) for the modified massive three (2 + 1)‐dimensional (3D) Abelian two‐form gauge theory with a single pseudoscalar field. The latter field (having the negative kinetic term
S. K. Panja +3 more
wiley +1 more source
Probing non-standard neutrino interactions with supernova neutrinos at Hyper-K
Journal of High Energy Physics, 2020 Non-standard neutrino self interactions (NSSI) could be stronger than Fermi interactions. We investigate the ability to constrain these four-neutrino interactions by their effect on the flux of neutrinos originating from a galactic supernova.
Minjie Lei +2 more
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Nonstandard neutrino interactions in supernovae
Physical Review D, 2016 Nonstandard interactions (NSI) of neutrinos with matter can significantly alter neutrino flavor evolution in supernovae with the potential to impact explosion dynamics, nucleosynthesis, and the neutrinos signal. In this paper, we explore, both numerically and analytically, the landscape of neutrino flavor transformation effects in supernovae due to NSI
Charles J. Stapleford +4 more
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Neutrino interactions in the deuterium-neon 14 foot double bubble chamber [PDF]
, 1970 V. E. Barnes +16 more
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Neutrino Opacity. II. Neutrino-Nucleon Interactions [PDF]
, 1964 John N. Bahcall, Steven C. Frautschi
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