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相关论文: A New Spin on Neutrino Quantum Kinetics

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We study spin and flavor oscillations of neutrinos under the influence of gravitational waves (GWs). We rederive the quasiclassical equation for the evolution of the neutrino spin in various external fields in curved spacetime starting from…

高能物理 - 唯象学 · 物理学 2020-01-22 Maxim Dvornikov

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…

A new approach is presented that treats NMR spin-spin relaxation as kinetics in spin phase space. The approach is applied to free induction decay (FID) in solids containing equivalent nuclear spins 1/2. The description obtained does not…

凝聚态物理 · 物理学 2009-10-30 Boris V. Fine

We have theoretically analyzed coherent nuclear-spin dynamics induced by electron transport through a quantum-dot spin valve. The hyperfine interaction between electron and nuclear spins in a quantum dot allows for the transfer of angular…

介观与纳米尺度物理 · 物理学 2015-06-23 Stefano Chesi , W. A. Coish

The phenomenon of neutrino oscillations is studied usually as a mixing between the flavor neutrinos and the neutrinos having a definite mass. The mixing angles and the mass eigenvalues are treated independently in order to accommodate the…

高能物理 - 唯象学 · 物理学 2013-03-27 A. Nicolaidis

Neutrino-neutrino interactions can lead to collective flavour conversion effects in supernovae and in the early universe. We demonstrate that the case of "bipolar" oscillations, where a dense gas of neutrinos and antineutrinos in equal…

天体物理学 · 物理学 2014-10-13 S. Hannestad , G. G. Raffelt , G. Sigl , Y. Y. Y. Wong

Neutrino flavor conversion is assumed to be induced by right-handed neutrino flavor conversion via seesaw mechanism. Neutrino oscillation is the macroscopic phenomenon before all neutrino flavor-flip interactions reaching equilibrium. The…

高能物理 - 唯象学 · 物理学 2022-10-18 Xiao-Yan Wang , Xiang-Jun Chen

The general formalism for the description of neutrino oscillations in arbitrary rapidly varying external fields is elaborated. We obtain the new effective Hamiltonian which determines the evolution of the averaged neutrino wave function.…

高能物理 - 唯象学 · 物理学 2016-12-07 Maxim Dvornikov

We develop a theoretical framework for quantum field description of neutrino evolution in a medium, with a focus on quantum decoherence induced by neutrino scattering on fermions. By deriving a generalized Lindblad master equation that…

高能物理 - 唯象学 · 物理学 2026-03-27 Konstantin Stankevich , Alexander Studenikin , Maksim Vyalkov

The dynamical spin susceptibility is studied in the magnetically-disordered phase of heavy-Fermion systems near the antiferromagnetic quantum phase transition. In the framework of the $S=1/2$ Kondo lattice model, we introduce a perturbative…

强关联电子 · 物理学 2009-10-31 C. Pepin , M. Lavagna

A new density matrix and corresponding quantum kinetic equations are introduced for fermions undergoing coherent evolution either in time (coherent particle production) or in space (quantum reflection). A central element in our derivation…

高能物理 - 唯象学 · 物理学 2009-02-02 Matti Herranen , Kimmo Kainulainen , Pyry Matti Rahkila

The origins of neutrino masses is one of the biggest mysteries in modern physics since they are beyond the realm of the Standard Model. As massive particles, neutrinos undergo flavor oscillations throughout their propagation. In this paper…

高能物理 - 唯象学 · 物理学 2024-09-04 Ivan Arraut , Enrique Arrieta-Diaz

Neutrino oscillations in the presence of strong gravitational fields are studied. We look at very high energy neutrinos ($\sim $1 TeV) emanating from Active Galactic Nuclei (AGN). It is observed that spin flavor resonant transitions of such…

高能物理 - 唯象学 · 物理学 2016-08-15 Dardo Píriz , Mou Roy , José Wudka

We argue that in at least a portion of the history of the universe the relic background neutrinos are spatially-extended, coherent superpositions of mass states. We show that an appropriate quantum mechanical treatment affects the neutrino…

天体物理学 · 物理学 2010-04-30 George M. Fuller , Chad T. Kishimoto

We all know that in the dense anisotropic interior of the star, neutrino-neutrino forward-scattering can lead to fast collective neutrino oscillations, which has striking consequences on flavor dependent neutrino emission and can be crucial…

高能物理 - 唯象学 · 物理学 2021-01-06 Soumya Bhattacharyya

Quantum gravity may involve models with stochastic fluctuations of the associated metric field, around some fixed background value. Such stochastic models of gravity may induce decoherence for matter propagating in such fluctuating space…

高能物理 - 唯象学 · 物理学 2009-07-22 Alexander Sakharov , Nick Mavromatos , Anselmo Meregaglia , Andre Rubbia , Sarben Sarkar

It is suggested that there is an underlying symmetry which relates the quark and lepton sectors. Namely, among the mixing matrix elements of CKM for quarks and PMNS for leptons there exist complementarity relations at a high energy scale…

高能物理 - 唯象学 · 物理学 2014-10-01 Hong-Wei Ke , Tan Liu , Xue-Qian Li

In the hot and dense medium of a supernova (SN) core, the nucleon spins fluctuate so fast that the axial-vector neutrino opacity and the axion emissivity are expected to be significantly modified. Axions with $m_a\alt10^{-2}\,{\rm eV}$ are…

天体物理学 · 物理学 2008-11-26 H. -T. Janka , W. Keil , G. Raffelt , D. Seckel

By means of nuclear spin-lattice relaxation rate 1/T1, we follow the spin dynamics as a function of the applied magnetic field in two gapped one-dimensional quantum antiferromagnets: the anisotropic spin-chain system NiCl2-4SC(NH2)2 and the…

We discuss an acceleration mechanism for pulsars out of their supernova remnants based on asymmetric neutrino emission from quark matter in the presence of a strong magnetic field. The polarized electron spin fixes the neutrino emission…

天体物理学 · 物理学 2008-11-26 I. Sagert , J. Schaffner-Bielich