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相关论文: A Magnetic Mass Model within the General Relativit…

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We thoroughly explore the cosmic gravitational focusing of cosmic neutrino fluid (C$\nu$F) by dark matter (DM) halo using both general relativity for a point source of gravitational potential and Boltzmann equations for continuous…

高能物理 - 唯象学 · 物理学 2024-07-08 Shao-Feng Ge , Pedro Pasquini , Liang Tan

Rainich-type conditions giving a spacetime "geometrization" of matter fields in general relativity are reviewed and extended. Three types of matter are considered: perfect fluids, scalar fields, and electromagnetic fields. Necessary and…

广义相对论与量子宇宙学 · 物理学 2015-07-22 D. S. Krongos , C. G. Torre

We model a compact relativistic body with anisotropic pressures in the presence of an electric field. The equation of state is barotropic with a linear relationship between the radial pressure and the energy density. Simple exact models of…

广义相对论与量子宇宙学 · 物理学 2015-06-17 P. Mafa Takisa , S. D. Maharaj

In the mean field approximation of the relativistic $\sigma$-$\omega$-$\rho$ model, the magnetic fields are incorporated, and its influence on the properties of n-p-e neutron star matter are studied. When the strength of the magnetic field…

天体物理学 · 物理学 2008-11-26 W. Chen , P. Q. Zhang , L. G. Liu

We derive an equation of state for magnetized charge neutral nuclear matter relevant for neutron star structure. The calculations are performed within an effective chiral model based on generalization of sigma model with nonlinear self…

核理论 · 物理学 2018-11-16 Tuhin Malik , Debashree Sen , T. K. Jha , Hiranmaya Mishra

The close vicinity of neutron stars remains poorly constrained by observations. Although plenty of data are available for the peculiar class of pulsars we are still unable to deduce the underlying plasma distribution in their magnetosphere.…

高能天体物理现象 · 物理学 2015-06-23 J. Pétri

Based on principles of the Expansive Nondecelerative Universe model that enables to quantify and localize the gravitational energy density, and stemming from the see-saw mechanism, the mass of electron, muon and tau neutrinos are determined…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Miroslav Sukenik , Jozef Sima

The extraordinary energetic activity of magnetars is usually explained in terms of dissipation of a huge internal magnetic field of the order of $10^{15-16}$G. How such a strong magnetic field can originate during the formation of a neutron…

高能天体物理现象 · 物理学 2017-07-26 A. G. Pili , N. Bucciantini , L. Del Zanna

We investigate the properties of the neutron star with relativistic mean field models. We incorporate in the quantum hadrodynamics and in the quark-meson coupling models a possible reduction of meson masses in nuclear matter. The equation…

核理论 · 物理学 2007-05-23 C. Y. Ryu , C. H. Hyun , S. W. Hong , B. K. Jennings

Bianchi type I massive string cosmological model with magnetic field of barotropic perfect fluid distribution through the techniques used by Latelier and Stachel, is investigated. To get the deterministic model of the universe, it is…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Raj Bali , Umesh Kumar Pareek , Anirudh Pradhan

Via a straightforward integration of the Einstein equations with cosmological constant, all static circularly symmetric perfect fluid 2+1 solutions are derived. The structural functions of the metric depend on the energy density, which…

广义相对论与量子宇宙学 · 物理学 2009-11-07 Alberto A. Garcia , Cuauhtemoc Campuzano

We determine the complete space-time metric from the bootstrapped Newtonian potential generated by a static spherically symmetric source in the surrounding vacuum. This metric contains post-Newtonian parameters which can be further used to…

广义相对论与量子宇宙学 · 物理学 2021-03-10 Roberto Casadio , Andrea Giusti , Iberê Kuntz , Giulio Neri

Aims. Many recent observations of pulsars and magnetars can be interpreted in terms of neutron stars (NS) with multipole electromagnetic fields. As a first approximation, we investigate the multipole magnetic and electric fields in the…

高能天体物理现象 · 物理学 2020-07-07 S. Bonazzola , F. Mottez , J. Heyvaerts

We obtain spacetimes generated by static and spinning magnetic string sources in Einstein Relativity with negative cosmological constant. Since the spacetime is asymptotically a cylindrical anti-de Sitter spacetime, we will be able to…

高能物理 - 理论 · 物理学 2009-11-07 Oscar J. C. Dias , Jose' P. S. Lemos

We investigate the causality and stability of the relativistic theory of magnetohydrodynamics derived in Phys. Rev. D 109, 096021 (2024) to describe a locally neutral two-component plasma of massless particles. We show that this formalism…

核理论 · 物理学 2025-05-16 Caio V. P. de Brito , Khwahish Kushwah , Gabriel S. Denicol

We define the center of mass and spin of an isolated system in General Relativity. The resulting relationships between these variables and the total linear and angular momentum of the gravitational system are remarkably similar to their…

广义相对论与量子宇宙学 · 物理学 2016-03-16 Carlos N. Kozameh , Gonzalo D. Quiroga

In this work we discuss different interpretations of mass in the relativistic dynamics. A new way to introduce mass is proposed. Our way is based on the relativistic equation of motion expressed in the form of the Newton$'$s second law. In…

经典物理 · 物理学 2018-03-22 V. A. Pletyukhov

Motivated by recent works on the origin of inertial mass, we revisit the relationship between the mass of charged particles and zero-point electromagnetic fields. To this end we first introduce a simple model comprising a scalar field…

高能物理 - 理论 · 物理学 2007-05-23 Giovanni Modanese

The concept of magnetic connections is extended to non-ideal relativistic magnetohydrodynamical plasmas. Adopting a general set of equations for relativistic magnetohydrodynamics including thermal-inertial, thermal electromotive, Hall and…

等离子体物理 · 物理学 2015-05-05 Felipe A. Asenjo , Luca Comisso

We reduce Einstein's field equations for the interior of a uniformly rotating, axisymmetric perfect fluid to a system of six second order partial differential equations for the pressure p the energy density $\mu$ and four dependent…

广义相对论与量子宇宙学 · 物理学 2016-08-31 E. Kyriakopoulos
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