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Combining the GW observations of merging systems of binary neutron stars and quasi-universal relations, we set constraints on the maximum mass that can be attained by nonrotating stellar models of neutron stars. More specifically,…

高能天体物理现象 · 物理学 2018-09-06 Luciano Rezzolla , Elias R. Most , Lukas R. Weih

The general scepticism and loss of faith on the predictive ability of different mass formulae, arising out of the divergence of their predictions in unknown regions taken with respect to a reference mass formula, is successfully dispelled.…

核理论 · 物理学 2007-05-23 S. K. Patra , P. Arumugam , L. Satpathy

In this work, we investigate the neutron star structure in conservative $f(R, T)$ gravity with $f(R, T)=R+\lambda T$, where $\lambda$ denotes the matter--geometry coupling. The modified stellar structure equations are solved using realistic…

宇宙学与河外天体物理 · 物理学 2026-01-27 Premachand Mahapatra , Prasanta Kumar Das

The gravitational wave signal from a binary neutron star merger carries the imprint of the deformability properties of the coalescing bodies, and then of the equation of state of neutron stars. In current models of the waveforms emitted in…

广义相对论与量子宇宙学 · 物理学 2022-07-20 Gonçalo Castro , Leonardo Gualtieri , Andrea Maselli , Paolo Pani

By extending our recent framework to describe the tidal deformations of a spinning compact object, we compute for the first time the tidal Love numbers of a spinning neutron star to linear order in the angular momentum. The spin of the…

广义相对论与量子宇宙学 · 物理学 2015-12-03 Paolo Pani , Leonardo Gualtieri , Valeria Ferrari

We study the deformation property of $\Lambda$ hypernuclei using the relativistic mean field (RMF) method. We find that $^{29}_{\Lambda}$Si and $^{13}_{\Lambda}$C hypernuclei have spherical shape as a consequence of the additional $\Lambda$…

核理论 · 物理学 2008-12-18 Myaing Thi Win , K. Hagino

We explore the constraints on dark sector models imposed by the recent observation of coincident gravitational waves and gamma rays from a binary neutron star merger, GW170817. Rather than focusing on specific models as has been considered…

宇宙学与河外天体物理 · 物理学 2018-07-26 Richard A. Battye , Francesco Pace , Damien Trinh

We have studied the effect of tidal deformability constraint given by the binary neutron star merger event GW170817 on the equations of state (EOS) of hybrid stars. The EOS are constructed by matching the hadronic EOS described by…

高能天体物理现象 · 物理学 2018-04-25 Rana Nandi , Prasanta Char

We systematically study the properties of pure nucleonic and hyperonic magnetic stars using a density-dependent relativistic mean field (DD-RMF) equations of state. We explore several parameter sets and hyperon coupling schemes within the…

核理论 · 物理学 2021-09-09 I. A. Rather , Usuf Rahaman , V. Dexheimer , A. A. Usmani , S. K. Patra

We use the Relativistic Mean Field (RMF) method to calculate properties of neutron rich, usually deformed nuclei, important for equation of state calculations and which have significant abundance in the early stages of stellar collapse. We…

天体物理学 · 物理学 2009-10-28 F. K. Sutaria , J. A. Sheikh , A. Ray

We report the recent progress in relativistic mean-field (RMF) and beyond approaches for the low-energy structure of deformed hypernuclei. We show that the $\Lambda$ hyperon with orbital angular momentum $\ell=0$ (or $\ell>1$) generally…

核理论 · 物理学 2019-09-04 J. M. Yao , H. Mei , K. Hagino , T. Motoba

We investigate the nonlinear tidal response of relativistic neutron stars by computing the fully relativistic, static, quadratic Love numbers. Using both the worldline effective field theory for extended gravitating bodies and second-order…

广义相对论与量子宇宙学 · 物理学 2025-12-17 Paolo Pani , Massimiliano Maria Riva , Luca Santoni , Nikola Savić , Filippo Vernizzi

Motivated by the unknown nature of the $2.50-2.67\,M_\odot$ compact object in the binary merger event GW190814, we study the maximum neutron star mass based on constraints from low-energy nuclear physics, neutron star tidal deformabilities…

核理论 · 物理学 2021-09-29 Yeunhwan Lim , Anirban Bhattacharya , Jeremy W. Holt , Debdeep Pati

On 17 August 2017, a gravitational wave event (GW170817) and an associated short gamma-ray burst (GRB 170817A) from a binary neutron star merger had been detected. The followup optical/infrared observations also identified the…

Relativistic mean field (RMF) theory of nuclear matter with the isovector scalar mean field corresponding to the delta-meson [a_0(980)] is studied. While the delta-meson mean field vanishes in symmetric nuclear matter, it can influence…

天体物理学 · 物理学 2009-10-30 S. Kubis , M. Kutschera

Observations of neutron-star mergers based on distinct messengers, including gravitational waves and electromagnetic signals, can be used to study the behavior of matter denser than an atomic nucleus, and to measure the expansion rate of…

高能天体物理现象 · 物理学 2020-12-22 Tim Dietrich , Michael W. Coughlin , Peter T. H. Pang , Mattia Bulla , Jack Heinzel , Lina Issa , Ingo Tews , Sarah Antier

We analyze the cosmology of the Randall-Sundrum model and that of compact brane models in general in the presence of a radius stabilization mechanism. We find that the expansion of our universe is generically in agreement with the expected…

高能物理 - 唯象学 · 物理学 2009-09-15 Csaba Csaki , Michael Graesser , Lisa Randall , John Terning

Subtracting the Strutinsky shell corrections from the selfconsistent energies obtained within the Relativistic Mean Field Theory (RMFT) we have got estimates for the macroscopic part of the binding energies of 142 spherical even-even…

核理论 · 物理学 2009-11-10 Bozena Nerlo-Pomorska , Joanna Sykut

The concordance (LambdaCDM) model reproduces the main current cosmological observations assuming the validity of general relativity at all scales and epochs, the presence of cold dark matter, and of a cosmological constant, equivalent to a…

宇宙学与河外天体物理 · 物理学 2018-11-08 Guido Risaliti , Elisabeta Lusso

This study evaluates the accuracy of nuclear fragmentation simulations using a quantum molecular dynamics (QMD) model based on relativistic mean field (RMF) theory for an energy range of 50-400 MeV/u, relevant to hadron therapy. A total of…