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Neutrino-neutrino refraction leads to collective flavor evolution that can include fast flavor conversion, an ingredient still missing in numerical simulations of core-collapse supernovae. We provide a theoretical framework for the linear…

高能物理 - 唯象学 · 物理学 2024-10-01 Damiano F. G. Fiorillo , Georg G. Raffelt

The flavor evolution of neutrinos in dense astrophysical sources, such as core-collapse supernovae or compact binary mergers, is non-linear due to the coherent forward scattering of neutrinos among themselves. Recent work in this context…

高能天体物理现象 · 物理学 2024-02-23 Marie Cornelius , Shashank Shalgar , Irene Tamborra

Dark Energy models are numerous and distinguishing between them is becoming difficult. However, using distinct observational probes can ease this quest and gives better assessment to the nature of Dark energy. To this end, the plausibility…

宇宙学与河外天体物理 · 物理学 2022-01-24 Ali Rida Khalifeh , Raul Jimenez

We consider the running of the neutrino mass matrix in the Standard Model and the Minimal Supersymmetric Standard Model, extended by heavy singlet Majorana neutrinos. Unlike previous studies, we do not assume that all of the heavy mass…

高能物理 - 唯象学 · 物理学 2015-06-25 Stefan Antusch , Joern Kersten , Manfred Lindner , Michael Ratz

We show that the Schr\"{o}dinger-Newton equation, which describes the nonlinear time evolution of self-gravitating quantum matter, can be made compatible with the no-signaling requirement by elevating it to a stochastic differential…

量子物理 · 物理学 2015-02-11 Stefan Nimmrichter , Klaus Hornberger

A theory of electromagnetic wave propagation in a weakly anisotropic smoothly inhomogeneous medium is developed, based on the quantum-mechanical diagonalization procedure applied to Maxwell equations. The equations of motion for the…

光学 · 物理学 2008-11-26 K. Yu. Bliokh , D. Yu. Frolov , Yu. A. Kravtsov

It is shown that the processes of neutrino oscillations in a magnetic field can be consistently described in the framework of a new quantum field-theoretical approach without use of the neutrino flavor states. It is based on the Feynman…

高能物理 - 唯象学 · 物理学 2022-10-19 Vadim Egorov , Igor Volobuev

We derive an analytical description of neutrino oscillations in matter based on the Magnus exponential representation of the time evolution operator. Our approach is valid in a wide range of the neutrino energies and properly accounts for…

天体物理学 · 物理学 2008-11-26 A. D. Supanitsky , J. C. D'Olivo , G. Medina-Tanco

We investigate the importance of going beyond the mean-field approximation in the dynamics of collective neutrino oscillations. To expand our understanding of the coherent neutrino oscillation problem, we apply concepts from many-body…

高能物理 - 唯象学 · 物理学 2019-10-09 Michael J. Cervia , Amol V. Patwardhan , A. B. Balantekin , S. N. Coppersmith , Calvin W. Johnson

We derive an explicit expressions for geometric description of state manifold obtained from evolution governed by a three parameter family of Hamiltonians covering most cases related to real interacting two-qubit systems. We discuss types…

量子物理 · 物理学 2019-06-12 Andrzej M. Frydryszak , Maria Gieysztor , Andrij Kuzmak

We consider the decoherence effects in the propagation of active neutrinos due to the non-forward neutrino scattering processes in a matter background composed of electrons and nucleons. We calculate the contribution to the imaginary part…

高能物理 - 唯象学 · 物理学 2021-07-07 José F. Nieves , Sarira Sahu

In dense neutrino environments, such as provided by core-collapse supernovae or neutron-star mergers, neutrino angular distributions may be unstable to collective flavor conversions, whose outcome remains to be fully understood. These…

高能物理 - 唯象学 · 物理学 2025-01-08 Damiano F. G. Fiorillo , Georg G. Raffelt

We show that flavor evolution of a system of neutrinos with continuous energy spectra as in supernovae can be understood in terms of the response of individual neutrino flavor-isospins (NFIS's) to the mean field. In the case of a system…

太阳与恒星天体物理 · 物理学 2011-08-12 Meng-Ru Wu , Yong-Zhong Qian

We re-examine the evolution of neutrino asymmetries in several four neutrino models. The first case involves the direct creation of $L_{\nu_e}$ by $\nu_e \leftrightarrow \nu_s$ oscillations. In the second case, we consider the mass…

高能物理 - 唯象学 · 物理学 2009-10-31 R. Foot

Active--sterile neutrino oscillations provide a mechanism by which large differences in the neutrino and antineutrino number densities can be created in the early universe. The quantum kinetic equations are employed in the study of these…

高能物理 - 唯象学 · 物理学 2009-10-31 Yvonne Y. Y. Wong

A new code for following the evolution and emissions of proto-neutron stars during the first minute of their lives is developed and tested. The code is one dimensional, fully implicit, and general relativistic. Multi-group, multi-flavor…

高能天体物理现象 · 物理学 2015-06-05 Luke F. Roberts

This paper presents a novel formalism for the out of equilibrium dynamics of the density matrix, capable of describing highly entangled many-body interactions. The evolution of quantum states is evaluated via eigenvalue dynamics of a…

量子物理 · 物理学 2025-10-28 Mumnuna Aziz Qureshi

We consider the time evolution of systems in which a spatially homogeneous scalar field is coupled to fermions. The quantum back-reaction is taken into account in one-loop approximation. We set up the basic equations and their…

高能物理 - 唯象学 · 物理学 2016-09-06 Juergen Baacke , Katrin Heitmann , Carsten Patzold

We study neutrino oscillations in space within a realistic model in which both the source and the target are considered to be stationary having Gaussian-form localizations. The model admits an exact analytic solution in field theory which…

高能物理 - 唯象学 · 物理学 2009-10-31 Ara Ioannisian , Apostolos Pilaftsis

A wrong derivation of the phase of a propagating massive particle which has repeatedly appeared during the last years has the advantage of leading once more to the important question of the phase difference between the mass eigenstates…

高能物理 - 唯象学 · 物理学 2009-01-06 Jean-Michel Levy