Zobrazeno 1 - 10
of 58
pro vyhledávání: '"Patwardhan, Amol V."'
In the presence of anisotropic neutrino and antineutrino fluxes, the quantum kinetic equations drive coherent oscillations in neutrino helicity, frequently referred to as spin oscillations. These oscillations depend directly on the absolute mass scal
Externí odkaz:
http://arxiv.org/abs/2404.08159
Autor:
Laber-Smith, Caroline, Armstrong, Eve, Balantekin, A. Baha, Jones, Elizabeth K., Newkirk, Lily, Patwardhan, Amol V., Ranginwala, Sarah, Sanchez, M. Margarette, Torres, Hansen
Publikováno v:
Phys. Rev. D, 110(4), 043011 (2024)
Understanding the physics of the deep solar interior, and the more exotic environs of core-collapse supernovae (CCSN) and binary neutron-star (NS) mergers, is of keen interest in many avenues of research. To date, this physics is based largely on sim
Externí odkaz:
http://arxiv.org/abs/2404.06468
We present a mechanism for producing a cosmologically-significant relic density of one or more sterile neutrinos. This scheme invokes two steps: First, a population of "heavy" sterile neutrinos is created by scattering-induced decoherence of active n
Externí odkaz:
http://arxiv.org/abs/2402.13878
The origin of the solar system abundances of several proton-rich isotopes, especially $^{92,94}$Mo and $^{96,98}$Ru, has been an enduring mystery in nuclear astrophysics. An attractive proposal to solve this problem is the $\nu p$-process, which can
Externí odkaz:
http://arxiv.org/abs/2312.03208
Publikováno v:
The Astrophysical Journal, 2024, Volume 967, Issue 2, id.146, 20 pp. The Astrophysical Journal, Volume 967, Issue 2, id.146, 20 pp
In high-energy astrophysical processes involving compact objects, such as core-collapse supernovae or binary neutron star mergers, neutrinos play an important role in the synthesis of nuclides. Neutrinos in these environments can experience collectiv
Externí odkaz:
http://arxiv.org/abs/2311.02562
Publikováno v:
Eur. Phys. J. A 59, 186 (2023)
In extreme astrophysical environments such as core-collapse supernovae and binary neutron star mergers, neutrinos play a major role in driving various dynamical and microphysical phenomena, such as baryonic matter outflows, the synthesis of heavy ele
Externí odkaz:
http://arxiv.org/abs/2305.01150
Publikováno v:
In: Handbook of Nuclear Physics (2022), Springer Nature, Singapore, edited by Tanihata, I., Toki, H., Kajino, T
Neutrino flavor transformations in core-collapse supernovae and binary neutron star mergers represent a complex and unsolved problem that is integral to our understanding of the dynamics and nucleosynthesis in these environments. The high number dens
Externí odkaz:
http://arxiv.org/abs/2301.00342
Autor:
Laber-Smith, Caroline, Ahmetaj, A. A., Armstrong, Eve, Balantekin, A. Baha, Patwardhan, Amol V., Sanchez, M. Margarette, Wong, Sherry
We continue examining statistical data assimilation (SDA), an inference methodology, to infer solutions to neutrino flavor evolution, for the first time using real - rather than simulated - data. The model represents neutrinos streaming from the Sun'
Externí odkaz:
http://arxiv.org/abs/2210.10884
The flavor evolution of neutrinos in environments with large neutrino number densities is an open problem at the nexus of astrophysics and neutrino flavor physics. Among the many unanswered questions pertaining to this problem, it remains to be deter
Externí odkaz:
http://arxiv.org/abs/2205.09384
Autor:
Cervia, Michael J., Siwach, Pooja, Patwardhan, Amol V., Balantekin, A. B., Coppersmith, S. N., Johnson, Calvin W.
Publikováno v:
Phys. Rev. D 105, 123025 (2022)
If a system of flavor-oscillating neutrinos is at high enough densities that neutrino-neutrino coherent forward scatterings are non-negligible, the system becomes a time-dependent many-body problem. An important and open question is whether the flavo
Externí odkaz:
http://arxiv.org/abs/2202.01865