Binding energy and stability of a cold neutron star

1978 ◽  
Vol 225 ◽  
pp. 708 ◽  
Author(s):  
I. Goldman ◽  
N. Rosen
Keyword(s):  
Neutron Star ◽  
Binding Energy ◽  
Cold Neutron

The maximum mass of a cold neutron star

1975 ◽  
Vol 202 ◽  
pp. 782 ◽  
Author(s):  
J. Rosen ◽  
N. Rosen
Keyword(s):  
Neutron Star ◽  
Cold Neutron ◽  
Maximum Mass

scholarly journals A cold neutron star in the transient low-mass X-ray binary HETE J1900.1–2455 after 10 yr of active accretion

2016 ◽  
Vol 465 (1) ◽  
pp. L10-L14 ◽  
Author(s):  
N. Degenaar ◽  
L.S. Ootes ◽  
M.T. Reynolds ◽  
R. Wijnands ◽  
D. Page
Keyword(s):  
Neutron Star ◽  
Cold Neutron ◽  
X Ray ◽  
Low Mass

scholarly journals Measuring the neutron star compactness and binding energy with supernova neutrinos

2017 ◽  
Vol 2017 (11) ◽  
pp. 036-036 ◽  
Author(s):  
Andrea Gallo Rosso ◽  
Francesco Vissani ◽  
Maria Cristina Volpe
Keyword(s):  
Neutron Star ◽  
Binding Energy ◽  
Supernova Neutrinos

EFFECTS OF IN-MEDIUM MODIFICATION OF WEAKLY INTERACTING LIGHT BOSON MASS IN NEUTRON STARS

2011 ◽  
Vol 26 (05) ◽  
pp. 367-375 ◽  
Author(s):  
A. SULAKSONO ◽  
MARLIANA ◽  
KASMUDIN
Keyword(s):  
Neutron Star ◽  
Binding Energy ◽  
Neutron Stars ◽  
Nuclear Matter ◽  
Observational Data ◽  
Boson Mass ◽  
Characteristic Scale ◽  
Neutron Star Matter ◽  
Weakly Interacting ◽  
Medium Modification

The effects of the presence of weakly interacting light boson (WILB) in neutron star matter have been revisited. Direct checking based on the experimental range of symmetric nuclear matter binding energy1 and the fact that the presence of this boson should give no observed effect on the crust properties of neutron star matter, shows that the characteristic scale of WILB [Formula: see text] should be ≤2 GeV-2. The recent observational data with significant low neutron stars radii2 and the recent largest pulsar which has been precisely measured, i.e. J1903+0327 (Ref. 3) indicate that in-medium modification of WILB mass in neutron stars cannot be neglected.

scholarly journals Analysis of Neutrino Burst from the Supernova in the Large Magellanic Cloud

1988 ◽  
Vol 108 ◽  
pp. 424-425
Author(s):  
Hideyuki Suzuki ◽  
Katsuhiko Sato
Keyword(s):  
Black Hole ◽  
Neutron Star ◽  
Binding Energy ◽  
Massive Star ◽  
Compact Object ◽  
Supernova Explosion ◽  
Large Magellanic Cloud ◽  
Magellanic Cloud

A massive star has been believed to end his life with the collapsed driven supernova explosion and the formation of the compact object such as a neutron star or a black hole. When the compact object is formed, a large amount of energy corresponding to the binding energy of the object must be released. It has been considered that most of the energy is emitted by neutrinos because of their adequate coupling with the matter. The observation of the neutrino burst from SN1987A by Kamiokande and IMB offered us the first chance to test these scenarios of the collapse driven supernova explosion directly. We began to analyze the data just after their publication and got many important results which are presented below. In our analysis the distance of SN1987A is assumed to be 50kpc.

scholarly journals Formation of Nuclear "Pasta" in Cold Neutron Star Matter

2003 ◽  
Vol 110 (4) ◽  
pp. 847-848 ◽  
Author(s):  
K. Iida ◽  
G. Watanabe ◽  
K. Sato
Keyword(s):  
Neutron Star ◽  
Cold Neutron ◽  
Neutron Star Matter

scholarly journals The decompression of cold neutron star matter

1977 ◽  
Vol 213 ◽  
pp. 225 ◽  
Author(s):  
J. M. Lattimer ◽  
F. Mackie ◽  
D. G. Ravenhall ◽  
D. N. Schramm
Keyword(s):  
Neutron Star ◽  
Cold Neutron ◽  
Neutron Star Matter
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