Results 91 to 100 of about 279,601 (204)

An updated nuclear-physics and multi-messenger astrophysics framework for binary neutron star mergers. [PDF]

Nat Commun, 2023
Pang PTH, Dietrich T, Coughlin MW, Bulla M, Tews I, Almualla M, Barna T, Kiendrebeogo RW, Kunert N, Mansingh G, Reed B, Sravan N, Toivonen A, Antier S, VandenBerg RO, Heinzel J, Nedora V, Salehi P, Sharma R, Somasundaram R, Van Den Broeck C.   +20 more
europepmc   +1 more source

The Black Hole Remnant of Black Hole-Neutron Star Coalescing Binaries

, 2013
We present a model for determining the dimensionless spin parameter and mass of the black hole remnant of black hole-neutron star mergers with parallel orbital angular momentum and initial black hole spin.
Pannarale, Francesco
core   +2 more sources

Neutrino transport in general relativistic neutron star merger simulations. [PDF]

Living Rev Comput Astrophys, 2023
Foucart F.
europepmc   +1 more source

Recent Developments on Kaon Condensation and Its Astrophysical Implications

, 2008
We discuss three different ways to arrive at kaon condensation at n_c = 3 n_0 where n_0 is nuclear matter density: (1) Fluctuating around the n=0 vacuum in chiral perturbation theory, (2) fluctuating around n_VM near the chiral restoration density n_chi ...
Brown, Gerald E., Lee, Chang-Hwan, Rho, Mannque   +2 more
core   +1 more source

Symmetry energy constraints from GW170817 and laboratory experiments

Physics Letters B, 2019
The LIGO-Virgo collaboration detection of the binary neutron-star merger event, GW170817, has expanded efforts to understand the Equation of State (EoS) of nuclear matter.
M.B. Tsang, W.G. Lynch, P. Danielewicz, C.Y. Tsang   +3 more
doaj  

Constraining neutron-star matter with microscopic and macroscopic collisions. [PDF]

Nature, 2022
Huth S, Pang PTH, Tews I, Dietrich T, Le Fèvre A, Schwenk A, Trautmann W, Agarwal K, Bulla M, Coughlin MW, Van Den Broeck C.   +10 more
europepmc   +1 more source

The Milky Way - Pulsars and Isolated Neutron Stars [PDF]

arXiv, 2002
CONTENTS The Milky Way -- Pulsars and Isolated Neutron Stars / Introduction: Historical Overview / Physics and Astrophysics of Isolated Neutron Stars / Rotation-powered Pulsars: The Magnetic Braking Model / High-energy Emission Models / Magnetospheric Emission Models / Thermal Evolution of Neutron Stars / Photospheric Emission from Cooling Neutron ...
arxiv  

High-Density Behavior and Dynamical Stability of Neutron Star Models. [PDF]

, 1964
C. W. Misner, H. S. Zapolsky
openalex   +1 more source

Neutron star mass estimates from gamma-ray eclipses in spider millisecond pulsar binaries. [PDF]

Nat Astron, 2023
Clark CJ, Kerr M, Barr ED, Bhattacharyya B, Breton RP, Bruel P, Camilo F, Chen W, Cognard I, Cromartie HT, Deneva J, Dhillon VS, Guillemot L, Kennedy MR, Kramer M, Lyne AG, Sánchez DM, Nieder L, Phillips C, Ransom SM, Ray PS, Roberts MSE, Roy J, Smith DA, Spiewak R, Stappers BW, Tabassum S, Theureau G, Voisin G.   +28 more
europepmc   +1 more source

Crust cooling curves of accretion-heated neutron stars [PDF]

arXiv, 2004
We discuss the recent efforts to use a sub-class of neutron-star X-ray transients (the quasi-persistent transients) to probe the properties of neutron-star crusts and cores. Quasi-persistent X-ray transients experience accretion episodes lasting years to decades, instead of the usual weeks to months of ordinary, short-duration transients.
arxiv