Results 111 to 120 of about 123,440 (246)

Gravitational-wave luminosity of binary neutron stars mergers

, 2017
We study the gravitational-wave peak luminosity and radiated energy of quasicircular neutron star mergers using a large sample of numerical relativity simulations with different binary parameters and input physics.
Bernuzzi, Sebastiano, Dietrich, Tim, Perego, Albino, Radice, David, Zappa, Francesco   +4 more
core   +1 more source

Strangeness in Neutron Stars

EPJ Web of Conferences
In this contribution I briefly review the dynamics of strange mesons and baryons with dense nuclear matter, paying a special attention to their pres ence in the inner core of neutron stars and the consequences for the structure of these compact stars.
openaire   +4 more sources

The neutron star zoo

Frontiers of Physics, 2013
15 pages, 8 figure, to be published in Frontiers of ...
openaire   +3 more sources

Detecting axion stars with radio telescopes

Physics Letters B, 2018
When axion stars fly through an astrophysical magnetic background, the axion-to-photon conversion may generate a large electromagnetic radiation power.
Yang Bai, Yuta Hamada
doaj   +1 more source

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

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

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

The crust of neutron stars [PDF]

AIP Conference Proceedings, 2007
The structure of the crust of a neutron star is completely determined by the experimentally measured nuclear masses up to a density of the order of 10^11 g.cm^{-3}. At higher densities, the composition of the crust still remains uncertain, mainly due to the presence of ``free'' superfluid neutrons which affect the properties of the nuclear ``clusters''.
openaire   +3 more sources

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

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

Neutron Stars and the EOS [PDF]

Proceedings of 8th International Workshop on Critical Point and Onset of Deconfinement — PoS(CPOD 2013), 2013
8 pages, 4 figures, 8th International Workshop on Critical Point and Onset of Deconfinement, To appear in Proceedings of ...
openaire   +2 more sources

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