scholarly journals Mass measurements of neutron rich isotopes in the Fe region and electron capture processes in neutron star crusts

2011 ◽  
Author(s):  
Alfredo Estrade ◽  
Milan Matos ◽  
Hendrik Schatz ◽  
Matthew Amthor ◽  
Mary Beard ◽  
...  
1990 ◽  
Vol 337 (4) ◽  
pp. 361-366 ◽  
Author(s):  
X. L. Tu ◽  
X. G. Zhou ◽  
D. J. Vieira ◽  
J. M. Wouters ◽  
Z. Y. Zhou ◽  
...  

1991 ◽  
Vol 260 (3-4) ◽  
pp. 285-290 ◽  
Author(s):  
X.G. Zhou ◽  
X.L. Tu ◽  
J.M. Wouters ◽  
D.J. Vieira ◽  
K.E.G. Löbner ◽  
...  

2019 ◽  
Vol 886 (1) ◽  
pp. L20 ◽  
Author(s):  
Thomas M. Tauris ◽  
Hans-Thomas Janka

2019 ◽  
Vol 100 (1) ◽  
Author(s):  
P. Ascher ◽  
N. Althubiti ◽  
D. Atanasov ◽  
K. Blaum ◽  
R. B. Cakirli ◽  
...  

Nature ◽  
2013 ◽  
Vol 505 (7481) ◽  
pp. 62-65 ◽  
Author(s):  
H. Schatz ◽  
S. Gupta ◽  
P. Möller ◽  
M. Beard ◽  
E. F. Brown ◽  
...  

2016 ◽  
Vol 31 (02n03) ◽  
pp. 1641017
Author(s):  
D. G. Yakovlev

General Relativity affects all major aspects of neutron star structure and evolution including radiation from the surface, neutron star models, evolution in compact binaries. It is widely used for neutron star mass measurements and for studying properties of superdense matter in neutron stars. Observations of neutron stars help testing General Relativity and planning gravitational wave experiments. No deviations from Einstein Theory of Gravity have been detected so far from observations of neutron stars.


2017 ◽  
Vol 13 (S337) ◽  
pp. 146-149 ◽  
Author(s):  
Robert D. Ferdman ◽  

AbstractPSR J1913+1102 is a double neutron star system (DNS) discovered in the Pulsar Arecibo L-band Feed Array survey. We have now very precisely measured the rate of advance of periastron for the system and the Einstein delay. From general relativity, this results in precise mass measurements: 1.65 ± 0.05 and 1.24 ± 0.05 M⊙ for the pulsar and neutron-star companion, respectively. This makes PSR J1913+1102 both the most massive double neutron star system known, and the most asymmetric in mass among compact DNS binaries. This asymmetry will allow for stringent limits on the effects of dipolar gravitational-wave radiation, predicted by alternative theories of gravity, as well as insight into heavy-element production from the eventual merger of this system and others like it. Further observations will also tighten constraints on formation and evolution models; this is crucial for understanding the DNS population, for which there are relatively few mass measurements.


1999 ◽  
Vol 512 (1) ◽  
pp. 288-299 ◽  
Author(s):  
S. E. Thorsett ◽  
Deepto Chakrabarty

2010 ◽  
Author(s):  
Ana Delia Becerril Reyes ◽  
Sanjib S. Gupta ◽  
Hendrik Schatz ◽  
Karl Ludwig Kratz ◽  
Peter Möller

2010 ◽  
Author(s):  
Edward Brown ◽  
Sanjib S. Gupta ◽  
Hendrik Schatz ◽  
Peter Möller ◽  
Karl Ludwig Kratz

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