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The coherent oscillation of axionic fields naturally drives copious production of dark photon particles in the early universe, due to resonance and tachyonic enhancement. During the process, energy is abruptly transferred from the former to…

宇宙学与河外天体物理 · 物理学 2021-01-04 Ryo Namba , Motoo Suzuki

The polarization of electromagnetic waves in the presence of a gravitational wave is analyzed. The rotation of the polarization angle and the Stokes parameters are deduced. A possible application to the detection of stochastic background of…

广义相对论与量子宇宙学 · 物理学 2016-02-03 Shahen Hacyan

Einstein-Cartan gravity is a close historical sibling of general relativity that allows for spacetime torsion. As a result, angular momentum couples to spacetime geometry in a similar way to energy. While consequences of this are well…

广义相对论与量子宇宙学 · 物理学 2024-12-17 Cédric Jockel , Leon Menger

We numerically calculate equilibrium configurations of uniformly rotating and charged neutron stars, in the case of insulating material and neglecting the electromagnetic forces acting on the equilibrium of the fluid. This allows us to…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Jerome Novak , Emmanuel Marcq

A galvanogyroscopic effect which is the rotational analog of the gravitomagnetic Hall effect has been proposed. As a consequence of Ohm's law in the rotating frame, the effect of the Coriolis force on the conduction current is predicted to…

其他凝聚态物理 · 物理学 2007-05-23 B. J. Ahmedov , M. J. Ermamatov

Gravitational waves (GW) are expected to interact with dark energy and dark matter, affecting their propagation on cosmological scales. In order to model this interaction, we derive a gauge invariant effective equation and action valid for…

宇宙学与河外天体物理 · 物理学 2024-03-29 Antonio Enea Romano

Rotation curves of spiral galaxies are known with reasonable precision for a large number of galaxies with similar morphologies. The data implies that non-Keplerian fall--off is seen. This implies that (i) large amounts of dark matter must…

天体物理学 · 物理学 2011-05-23 C. Rodrigo-Blanco , J. Pérez-Mercader

We present a detailed theoretical and experimental study of the rotation of the plane of polarization of light traveling through a gas of fast-spinning molecules. This effect is similar to the polarization drag phenomenon predicted by Fermi…

A rotating star's oblateness creates a deformation in the gravitational field outside the star, which is measured by the quadrupole-moment tensor. We consider the effect of the quadrupole moment on the orbital motion and rate of inspiral of…

广义相对论与量子宇宙学 · 物理学 2016-08-25 Eric Poisson

We calculate the gravitational radiation produced by the coalescence of inspiraling binary neutron stars in the Newtonian regime using 3-dimensional numerical simulations. The stars are modeled as polytropes and start out in the point-mass…

广义相对论与量子宇宙学 · 物理学 2011-09-09 Xing Zhuge , Joan M. Centrella , Stephen L. W. McMillan

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

A new theory for the dynamics of the magnetic particles and their magnetic moments in ferrofluids is developed. Based on a generalized Lagrangian formulation for the equations of motion of the colloidal particle, we introduce its…

统计力学 · 物理学 2007-05-23 Claudio Scherer , Hans-Georg Matuttis

We establish thermodynamic stability and gauge invariance in the magnetovortical matter of Dirac fermions under the coexistent rotation and strong magnetic field. The corresponding partition function reveals that the orbital contribution to…

高能物理 - 唯象学 · 物理学 2025-07-02 Kenji Fukushima , Koichi Hattori , Kazuya Mameda

Spinning neutron stars, when observed as pulsars, are seen to undergo occasional spin-up events known as glitches. Despite several decades of study, the physical mechanisms responsible for glitches are still not well understood, but…

高能天体物理现象 · 物理学 2024-01-09 Brynmor Haskell , David Ian Jones

This paper proposes a strategy for detecting the presence of a gravito-magnetic field due to the rotation of the galactic dark halo. Visible matter in galaxies rotates and dark matter, supposed to form a halo incorporating barionic matter,…

广义相对论与量子宇宙学 · 物理学 2018-12-19 Angelo Tartaglia

A la Pontecorvo when one defines electroweak flavour states of neutrinos as a linear superposition of mass eigenstates one ignores the associated spin. If, however, there is a significant rotation between the neutrino source, and the…

高能物理 - 唯象学 · 物理学 2013-02-21 D. V. Ahluwalia , Cheng-Yang Lee

We compute the energy spectra of the gravitational signals emitted when a pointlike mass moves on a closed orbit around a non rotating neutron star, inducing a perturbation of its gravitational field and its internal structure. The Einstein…

广义相对论与量子宇宙学 · 物理学 2009-11-07 L. Gualtieri , E. Berti , J. A. Pons , G. Miniutti , V. Ferrari

The first-order gravity effects of Dirac wave functions are found from the inertial effects in the accelerated frames of reference. Derivations and discussions about Lense-Thirring effect and the gyrogravitational ratio for intrinsic spin…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Yi-Cheng Huang , Wei-Tou Ni

We show that the Standard Model electroweak interaction of ultrarelativistic electrons with nucleons ($eN$ interaction) in a neutron star (NS) permeated by a seed large-scale helical magnetic field provides its growth up to $\gtrsim…

高能天体物理现象 · 物理学 2016-08-10 Maxim Dvornikov , Victor B. Semikoz

Recent theoretical work has shown that spin $1/2$ particles moving through unpolarized matter which sources torsion fields experience a new type of parity-even and time-reversal-odd optical potential if the matter is spinning in the lab…

核实验 · 物理学 2017-01-04 A. N. Ivanov , W. M. Snow