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相关论文: The influence of quantum vacuum friction on pulsar…

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Magnetars are proposed to be peculiar neutron stars which could power their X-ray radiation by super-strong magnetic fields as high as $\gtrsim 10^{14}$ G. However, no direct evidence for such strong fields is obtained till now, and the…

高能天体物理现象 · 物理学 2016-01-20 Xue-Yu Xiong , Chun-Yuan Gao , Ren-Xin Xu

In this letter we show that Quantum Vacuum Friction (QVF) should play an important role in neutron star evolution. Taking into account this effect we show that magnetars could be understood as a natural evolution of standard pulsars. For…

太阳与恒星天体物理 · 物理学 2010-10-06 Arnaud Dupays , Carlo Rizzo , Bignami Giovanni Fabrizio

The energy loss of a rotationally powered pulsar is primarily carried away as electromagnetic radiation and a particle wind. Considering that the magnetic field strength of pulsars ranges from about $10^8$ to $10^{15}$ G, one could expect…

高能天体物理现象 · 物理学 2019-04-24 Paul Ripoche , Jeremy Heyl

In this letter we calculate the energy loss of highly magnetized neutron star due to friction with quantum vacuum, namely Quantum Vacuum Friction (QVF). Taking into account one-loop corrections in the effective Heisenberg-Euler Lagrangian…

天体物理学 · 物理学 2009-06-23 Arnaud Dupays , Carlo Rizzo , Dimitar Bakalov , Giovanni F. Bignami

The topology of the electromagnetic field around neutron stars severely impacts pulsar physics. While most of the works assume a standard centred dipolar magnetic field model, recently some efforts have been made to explain how inclusion of…

高能天体物理现象 · 物理学 2017-07-27 Anu Kundu , Jerome Petri

The aim of this article is to draw attention to the importance of the electric current loss in the energy output of radio pulsars. We remind that even the losses attributed to the magneto-dipole radiation of a pulsar in vacuum can be…

天体物理学 · 物理学 2008-11-26 V. S. Beskin , E. E. Nokhrina

It is shown that depletion of the magnetic field pressure in a quaking neutron star undergoing Lorentz-force-driven torsional seismic vibrations about axis of its dipole magnetic moment is accompanied by the loss of vibration energy of the…

高能天体物理现象 · 物理学 2010-09-07 S. I. Bastrukov , I. V. Molodtsova , J. W. Yu , R. X. Xu

Most studies of the pulsar magnetosphere have assumed a pure magnetic dipole in flat spacetime. However, recent work suggests that the effects of general relativity are in fact of vital importance and that realistic pulsar magnetic fields…

高能天体物理现象 · 物理学 2016-12-21 Samuel E. Gralla , Alexandru Lupsasca , Alexander Philippov

Pulsars are good clocks in the universe. One fundamental question is that why they are good clocks? This is related to the braking mechanism of pulsars. Nowadays pulsar timing is done with unprecedented accuracy. More pulsars have braking…

高能天体物理现象 · 物理学 2016-01-14 H. Tong

In juxtaposition with the standard model of rotation powered pulsar, the model of vibration powered magnetar undergoing quake-induced torsional Alfven vibrations in its own ultra strong magnetic field experiencing decay is considered. The…

高能天体物理现象 · 物理学 2015-03-19 S. Bastrukov , J. W. Yu , R. X. Xu , I. Molodtsova

The aim of this article is to draw attention to the importance of the electric current loss in the energy output of radio pulsars. We remind that even the losses attributed to the magneto-dipole radiation of a pulsar in vacuum can be…

天体物理学 · 物理学 2007-05-23 V. S. Beskin , E. E. Nokhrina

A fascinating effect belonging to the field of vacuum forces and fluctuations is that of quantum friction. It refers to the prediction of a dissipative force acting on a moving object due to the quantum vacuum field. In this work, we…

量子物理 · 物理学 2026-02-17 Nicolas Schüler , O. J. Franca , Michael Vaz , Hervé Bercegol , Stefan Yoshi Buhmann

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

It is common practice to take for granted the equality (up to the constant $\varepsilon_0$) of the electric displacement ($\bf{D}$) and electric ($\bf{E}$) field vectors in vacuum. The same happens with the magnetic field ($\bf{H}$) and the…

广义相对论与量子宇宙学 · 物理学 2023-07-14 Sébastien Fumeron , Fernando Moraes , Bertrand Berche

The energy-loss formula of the production of gravitons by the binary is derived in the source theory formulation of gravity. Then, the quantum energy-loss formula involving radiative corrections is derived. We postulate an idea that…

高能物理 - 唯象学 · 物理学 2007-05-23 Miroslav Pardy

Pulsar braking torques due to magnetodipole radiation and to unipolar generator are considered, which results in braking index being less than 3 and could be employed to test the emission models. Improved equations to obtain pulsar braking…

天体物理学 · 物理学 2009-11-07 R. X. Xu , G. J. Qiao

We compute the characteristic parameters of magnetic dipole radiation of a neutron star undergoing torsional seismic vibrations under the action of Lorentz restoring force about axis of a dipolar magnetic field experiencing decay. After…

高能天体物理现象 · 物理学 2015-05-28 S. I. Bastrukov , R. X. Xu , J. W. Yu , I. V. Molodtsova

As demonstrated in our previous work [J. Chem. Phys. 149, 174109 (2018)], the kinetic energy imparted to a quantum rotor by a non-resonant electromagnetic pulse with a Gaussian temporal profile exhibits quasi-periodic drops as a function of…

量子物理 · 物理学 2021-12-22 Mallikarjun Karra , Bretislav Friedrich , Burkhard Schmidt

We study the response of the QCD vacuum to an external magnetic field, in the presence of strong CP violation. Using chiral perturbation theory and large N_c expansion, we show that the external field would polarize quantum fluctuations and…

高能物理 - 唯象学 · 物理学 2008-11-26 R. Millo , P. Faccioli

The magnetosphere of, and electromagnetic (EM) radiation from pulsars are usually described in the framework of classical electrodynamics. For some pulsars, however, whose emission heights are relatively close to the surface of the neutron…

高能天体物理现象 · 物理学 2021-09-29 Dong-Hoon Kim , Sascha Trippe
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