scholarly journals R-mode instability of strange stars and observations of neutron stars in LMXBs

2015 ◽  
Vol 15 (6) ◽  
pp. 871-878 ◽  
Author(s):  
Chun-Mei Pi ◽  
Shu-Hua Yang ◽  
Xiao-Ping Zheng
2019 ◽  
Vol 19 (2) ◽  
pp. 030 ◽  
Author(s):  
Yu-Bin Wang ◽  
Xia Zhou ◽  
Na Wang ◽  
Xiong-Wei Liu

2012 ◽  
Vol 8 (S291) ◽  
pp. 536-536
Author(s):  
Martin Urbanec ◽  
John Miller ◽  
Zdenek Stuchlik

AbstractWe present quadrupole moments of rotating neutron and strange stars calculated using standard Hartle Thorne approach. We demonstrate differences between neutron and strange star parameters connected with quadrupole moments and how this parameters could be, in the case of neutron stars, approximated almost independently on neutron star equation of state.


New Astronomy ◽  
2009 ◽  
Vol 14 (1) ◽  
pp. 37-39 ◽  
Author(s):  
Manjari Bagchi ◽  
Jishnu Dey ◽  
Sushan Konar ◽  
Gour Bhattacharya ◽  
Mira Dey
Keyword(s):  

2013 ◽  
Vol 433 (3) ◽  
pp. 1903-1909 ◽  
Author(s):  
M Urbanec ◽  
J. C Miller ◽  
Z Stuchlík

2001 ◽  
Vol 10 (04) ◽  
pp. 381-441 ◽  
Author(s):  
NILS ANDERSSON ◽  
KOSTAS D. KOKKOTAS

In this review we summarize the current understanding of the gravitational-wave driven instability associated with the so-called r-modes in rotating neutron stars. We discuss the nature of the r-modes, the detailed mechanics of the instability and its potential astrophysical significance. In particular we discuss results regarding the spin-evolution of nascent neutron stars, the detectability of r-mode gravitational waves and mechanisms limiting the spin-rate of accreting neutron stars in binary systems.


Sign in / Sign up

Export Citation Format

Share Document