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相关论文: Inverse beta-decay in magnetic fields

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In this work we explore the effects of a weak magnetic field on the decay process of a neutral scalar boson into a pair of charged fermions in vacuum. Since the analytical computation of the decay width needs of some approximation,…

高能物理 - 唯象学 · 物理学 2019-03-27 Jorge Jaber-Urquiza , Gabriella Piccinelli , Angel Sanchez

We consider random primordial magnetic fields and discuss their dissipation, coherence length $L_0$, scaling behaviour and constraints implied by the primoridal nucleosynthesis. Such magnetic fields could excite the right-helicity states of…

高能物理 - 唯象学 · 物理学 2011-07-19 Kari Enqvist , A. I. Rez , V. V. Semikoz

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 inverse solution of the 1D Parker dynamo equations is considered. The method is based on minimization of the cost-function, which characterize deviation of the model solution properties from the desired ones. The output is the latitude…

流体动力学 · 物理学 2015-11-20 M. Yu. Reshetnyak

Modelling as a dipole the magnetic interaction of a binary system of neutron stars, we are able to include the magnetic effects in the Newtonian and in the inspiral dynamics of the system using an equivalent one-body description.…

广义相对论与量子宇宙学 · 物理学 2022-11-30 Mariana Lira , Juan Carlos Degollado , Claudia Moreno , Darío Núñez

The potential enhancement of the cross section $\nu\bar\nu\to e^+e^-$ in the presence of a magnetic field is of critical interest for the study of supernovae and as a possible mechanism for gamma ray bursts. While parity violation(PV) in…

天体物理学 · 物理学 2007-05-23 C. J. Benesh , C. J. Horowitz

We ask the question of how angular momentum is conserved in electroweak interaction processes. To introduce the problem with a minimum of mathematics, we first raise the same issue in elastic scattering of a circularly polarized photon by…

高能物理 - 唯象学 · 物理学 2024-09-05 Gordon Baym , Jen-Chieh Peng , C. J. Pethick

Millisecond pulsars are rather weakly-magnetized neutron stars which are thought to have been spun up by disc accretion, with magnetic linkage between the star and the disc playing a key role. Their spin history depends sensitively on…

太阳与恒星天体物理 · 物理学 2013-10-28 L. Naso , W. Kluźniak , J. C. Miller

Theoretical predictions for the magnetic moments of the physical Delta baryons are extracted from lattice QCD calculations. We utilize finite-range regulated effective field theory that is constructed to have the correct Dirac moment mass…

高能物理 - 格点 · 物理学 2010-02-17 I. C. Cloet , D. B. Leinweber , A. W. Thomas

A consistent treatment of intrinsic and collective coordinates is applied to the calculation of matrix elements describing nuclear double beta decay transitions. The method, which was developed for the case of nuclear rotations, is adapted…

核理论 · 物理学 2009-10-31 D. R Bes , O. Civitarese , N. N. Scoccola

The recent discovery of the "weak field, old magnetar", the soft gamma repeater SGR 0418+5729, whose dipole magnetic field is less than 7.5 \times 10^{12} G, has raised perplexing questions: How can the neutron star produce SGR-like bursts…

高能天体物理现象 · 物理学 2015-05-30 S. Dall'Osso , J. Granot , T. Piran

The magnetic dipole transitions between the vector mesons $B_c^*$ and their relevant pseudoscalar mesons $B_c$ ($B_c$, $B_c^*$, $B_c(2S)$, $B_c^*(2S)$, $B_c(3S)$ and $B_c^*(3S)$ etc, the binding states of $(c\bar{b})$ system) of the $B_c$…

高能物理 - 唯象学 · 物理学 2011-01-28 Hong-Wei Ke , Guo-Li Wang , Xue-Qian Li , Chao-Hsi Chang

A detailed study of exchange-biased Fe/MnF2 bilayers using magneto-optical Kerr Effect shows that the magnetization reversal occurs almost fully through domain wall nucleation and propagation for external fields parallel to the exchange…

材料科学 · 物理学 2007-05-23 Elke Arenholz , Kai Liu

In this study, we model a pulsar as a general relativistic oblique rotator, where the oblique rotator is a rotationally deformed neutron star whose rotation and magnetic axis are inclined at an angle. The oblique rotator spins down, losing…

高能天体物理现象 · 物理学 2022-05-04 Sagnik Chatterjee , Ritam Mallick

We predict unidirectional magnetoresistance effects arising in a bilayer composed of a nonmagnetic metal and a ferromagnetic insulator, whereby both longitudinal and transverse resistances vary when the direction of the applied electric…

介观与纳米尺度物理 · 物理学 2025-03-10 M. Mehraeen , Pengtao Shen , Steven S. -L. Zhang

The anisotropy of the positrons emitted in the reaction $\bar{\nu}_{e}+p\to n+e^{+}$ has to be taken into account for extracting an antineutrino signal in Superkamiokande. For the Sun, this effect allows a sensitivity to…

天体物理学 · 物理学 2009-10-30 G. Fiorentini , M. Moretti , F. L. Villante

We compute the one-loop thermo-magnetic corrections to the self-coupling in a model where charged scalars interact also with a constant magnetic field. The calculation is motivated by the possibility that the critical temperature for the…

高能物理 - 唯象学 · 物理学 2014-08-13 Alejandro Ayala , M. Loewe , Ana Julia Mizher , R. Zamora

Spectroscopic studies of two beta-rays from 100Mo are shown to be of potential interest for investigating both the Majorana neutrino mass by neutrinoless double beta-decay and low energy solar neutrino's by inverse beta-decay. With a…

核实验 · 物理学 2009-10-31 H. Ejiri , J. Engel , R. Hazama , P. Krastev , N. Kudomi , R. G. H. Robertson

A multipole spin-down equation based on a monopolar term is derived from the general expression $\dot{\nu} = -f(\nu,t)$ and used to study pulsar evolution. We show that the time-independent version of such equation cannot reproduce the…

天体物理学 · 物理学 2009-11-10 Cesar Alvarez , Alberto Carramiñana