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相关论文: Galvano-rotational effect induced by electroweak i…

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The description of physical processes in accelerated frames opens a window to numerous new phenomena. One can encounter these effects both in the subatomic world and on a macroscale. In the present work we review our recent results on the…

高能物理 - 唯象学 · 物理学 2017-05-19 Maxim Dvornikov

We study the evolution of neutrinos electroweakly interacting with a rotating matter. The description of neutrinos is based on the Dirac equation in the corotating noninertial frame where matter is at rest. We find solution of this Dirac…

高能物理 - 唯象学 · 物理学 2026-03-25 Alexander Breev , Maxim Dvornikov

In this comment, we show that the fundamental equation worked by Dvornikov in his paper is incorrect, which is given by the Dirac equation for a neutrino interacting with matter in a rotating frame (or curved space-time). In particular,…

高能物理 - 唯象学 · 物理学 2025-09-24 R. R. S. Oliveira

In this paper, we discuss the impact of rotation on the particle composition of rotating neutron stars (pulsars). Particular emphasis is put on the formation of quark matter during stellar spin-down, driven by continuous gravitational…

高能天体物理现象 · 物理学 2017-09-06 R. D. Mellinger , F. Weber , W. Spinella , G. A. Contrera , M. Orsaria

We show that the spin of dark matter induces a gravitational analog of the electromagnetic Faraday effect, where the polarization of gravitational waves undergoes a rotation as they propagate through a dark matter halo with a non-vanishing…

广义相对论与量子宇宙学 · 物理学 2024-09-25 F. Barriga , F. Izaurieta , S. Lepe , P. Mesa , J. Muñoz , C. Quinzacara , O. Valdivia

We study the gravitational Faraday rotation, on linearly polarized light rays emitted by a pulsar, orbiting another compact object. We relate the rotation angle to the orbital phase of the emitting pulsar, as well as to other parameters…

天体物理学 · 物理学 2008-11-26 Matteo Luca Ruggiero , Angelo Tartaglia

New effects of nontrivial neutrino electromagnetic properties are investigated on the basis of exact solutions of the modified Dirac equations for neutrinos in dense magnetized rotating matter. The effect of spatial separation of different…

高能物理 - 唯象学 · 物理学 2014-06-11 Alexander Studenikin , Ilya Tokarev

The rotating relativistic fermion system is considered. The consideration is based on the Dirac equation written in the laboratory (non - rotating) reference frame. Rotation in this approach gives rise to the effective magnetic and electric…

高能物理 - 唯象学 · 物理学 2018-04-12 M. A. Zubkov

The origin of pulsar kicks is reviewed in the framework of the spin-flip conversion of neutrinos propagating in the gravitational field of a magnetized protoneutron star. We find that for a mass in rotation with angular velocity ${\bbox…

天体物理学 · 物理学 2009-11-10 G. Lambiase

Observations of short-duration gamma-ray bursts and their afterglows show that a good fraction (perhaps $\gtrsim50\%$) of binary neutron star mergers lead to strongly magnetized, rapidly rotating pulsars (including millisecond magnetars),…

高能天体物理现象 · 物理学 2019-02-22 Z. G. Dai

We study the evolution of neutrinos in a background matter moving with a linear acceleration. The Dirac equation for a massive neutrino electroweakly interacting with background fermions is obtained in a comoving frame where matter is at…

高能物理 - 唯象学 · 物理学 2015-09-03 Maxim Dvornikov

The proposition that dark matter halos possess angular momentum, though widely accepted, is a theoretical prediction which has, till date, not been observationally verified. The gravi-magnetic field produced by a rotating gravitating object…

天体物理学 · 物理学 2007-05-23 Partha Nag , Somnath Bharadwaj , Sayan Kar

The gravitational neutrino oscillation problem is studied by considering the Dirac Hamiltonian in a Riemann-Cartan space-time and calculating the dynamical phase. Torsion contributions which depend on the spin direction of the mass…

广义相对论与量子宇宙学 · 物理学 2010-12-23 M. Adak , T. Dereli , L. H. Ryder

We derive equations of motion for paramagnetic and ferromagnetic particles fully accounting for gyromagnetic effects. Considering the Einstein-de Haas effect for an ellipsoidal paramagnetic particle we find that starting from a quiescent…

软凝聚态物质 · 物理学 2023-10-24 M. Belovs , R. Livanovics , A. Cebers

The model for the generation of magnetic fields in a neutron star, based on the magnetic field instability caused by the electroweak interaction between electrons and nucleons, is developed. Using the methods of the quantum field theory,…

高能物理 - 唯象学 · 物理学 2017-01-12 Maxim Dvornikov

The origin of high velocities of pulsars is studied by considering the spin-flip conversion of neutrinos propagating in a gravitational field of a protoneutron star. For a rotating gravitational source (such as pulsars) with angular…

天体物理学 · 物理学 2015-06-24 G. Lambiase

We present quite a powerful method in investigations of different phenomena that can appear when neutrinos and electrons propagate in background matter. This method implies use of exact solutions of modified Dirac equations that contain the…

高能物理 - 唯象学 · 物理学 2008-11-26 Alexander Studenikin

Based on Maxwellian quaternionic electromagnetic theory, the electromagnetic interaction, gravitational interaction and their coupling influence with the dark matter field in octonionic space are discussed. The research results disclose the…

经典物理 · 物理学 2009-10-28 Zihua Weng

In this paper the interaction of high energy neutrinos with weak gravitational fields is briefly explored. The form of the graviton-neutrino vertex is motivated from Lorentz and gauge invariance and the non-relativistic interpretations of…

高能物理 - 唯象学 · 物理学 2008-12-30 A. Menon , Arun M. Thalapillil

We study neutrinos gravitationally scattered off a rotating supermassive black hole which is surrounded by a thin accretion disk with a realistic magnetic field. Neutrinos are supposed to be Dirac particles having a nonzero magnetic moment.…

高能物理 - 唯象学 · 物理学 2022-12-05 Maxim Dvornikov
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