Withdrawn as Duplicate: Neutron star crust cooling in KS 1731-260: the influence of accretion outburst variability on the crustal temperature evolution

2016 ◽  
Vol 485 (1) ◽  
pp. L16-L16
Author(s):  
Laura S Ootes ◽  
Dany Page ◽  
Rudy Wijnands ◽  
Nathalie Degenaar
Keyword(s):  
Neutron Star ◽  
Temperature Evolution ◽  
Neutron Star Crust

scholarly journals Moment of inertia of neutron star crust in alternative and modified theories of gravity

2016 ◽  
Vol 94 (2) ◽  
Author(s):  
Kalin V. Staykov ◽  
K. Yavuz Ekşi ◽  
Stoytcho S. Yazadjiev ◽  
M. Metehan Türkoğlu ◽  
A. Savaş Arapoğlu
Keyword(s):  
Neutron Star ◽  
Moment Of Inertia ◽  
Modified Theories Of Gravity ◽  
Neutron Star Crust ◽  
Theories Of Gravity

scholarly journals Shear viscosity in magnetized neutron star crust

2015 ◽  
Vol 112 (5) ◽  
pp. 59001 ◽  
Author(s):  
D. D. Ofengeim ◽  
D. G. Yakovlev
Keyword(s):  
Neutron Star ◽  
Shear Viscosity ◽  
Neutron Star Crust

scholarly journals Torsional shear oscillations in the neutron star crust driven by the restoring force of elastic stresses

2007 ◽  
Vol 382 (2) ◽  
pp. 849-859 ◽  
Author(s):  
S. I. Bastrukov ◽  
H.- K. Chang ◽  
J. Takata ◽  
G.- T. Chen ◽  
I. V. Molodtsova
Keyword(s):  
Neutron Star ◽  
Restoring Force ◽  
Elastic Stresses ◽  
Neutron Star Crust ◽  
Torsional Shear

scholarly journals Timing of Optical Pulses from the Crab Nebula Pulsar

1971 ◽  
Vol 46 ◽  
pp. 119-124
Author(s):  
P. E. Boynton ◽  
E. J. Groth ◽  
R. B. Partridge ◽  
David T. Wilkinson
Keyword(s):  
Neutron Star ◽  
Crab Nebula ◽  
Physical Models ◽  
Quiet Period ◽  
Eccentric Orbit ◽  
Optical Pulses ◽  
Neutron Star Crust ◽  
Alternate Explanation ◽  
Speed Up ◽  
The Crab Nebula

Timing the arrival of optical pulses from NP 0532 is a potentially important tool for studying the physics of this fascinating object. However, there are some difficulties in interpreting the data in terms of physical models. Some progress has been made on understanding the largest effect – the pulsar braking mechanism. The glitch of late September, 1969 can be interpreted as the speed-up, and subsequent relaxation, of the rotation of a neutron star crust. An alternate explanation is that of a planet in an eccentric orbit. Both models fit the rather meager data near the event. A small sinusoidal effect is indicated in a relatively quiet period of the data.

The r-process nucleosynthesis during the decompression of neutron star crust material

2014 ◽  
Author(s):  
S. Goriely ◽  
A. Bauswein ◽  
H.-T. Janka ◽  
J.-L. Sida ◽  
J.-F. Lemaı̂tre ◽  
...  
Keyword(s):  
Neutron Star ◽  
Neutron Star Crust ◽  
R Process
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