scholarly journals Constraints on scalar asymmetric dark matter from black hole formation in neutron stars

2012 ◽  
Vol 85 (2) ◽  
Author(s):  
Samuel D. McDermott ◽  
Hai-Bo Yu ◽  
Kathryn M. Zurek
2007 ◽  
Vol 24 (12) ◽  
pp. S207-S219 ◽  
Author(s):  
B C Stephens ◽  
M D Duez ◽  
Y T Liu ◽  
S L Shapiro ◽  
M Shibata

2014 ◽  
Vol 2014 ◽  
pp. 1-6 ◽  
Author(s):  
A. V. Grobov ◽  
S. G. Rubin ◽  
V. Yu. Shalamova

A mechanism of primordial black hole formation with specific mass spectrum is discussed. It is shown that these black holes could contribute to the energy density of dark matter. Our approach is elaborated in the framework of universal extra dimensions.


2009 ◽  
Vol 2009 (08) ◽  
pp. 024-024 ◽  
Author(s):  
Hideyuki Umeda ◽  
Naoki Yoshida ◽  
Ken'ichi Nomoto ◽  
Sachiko Tsuruta ◽  
Mei Sasaki ◽  
...  

1996 ◽  
Vol 165 ◽  
pp. 257-262
Author(s):  
D. A. Frail

If one is interested in issues related to the birth and evolution of neutron stars, a promising avenue of research begins with the study of the byproducts of a Type II supernova event, namely a pulsar (PSR) and its supernova remnant (SNR). However, it has long been a matter of some embarrassment that out of the more than 600 known PSRs and the 175 catalogued SNRs there are few associations. In fact, for nearly 15 years following the discovery of PSRs only the Crab and Vela PSRs had an associated remnant. This failure has spawned something of a cottage industry to “explain away” the low incidence of PSR/SNR associations. Beaming (Frail & Moffett 1993; Narayan & Schaudt 1988), injection (Narayan 1987), field growth (Blandford, Applegate & Hernquist 1983) and black-hole formation (Chevalier 1994) have been invoked in this context at one time or another.


2019 ◽  
Vol 485 (3) ◽  
pp. 3352-3359 ◽  
Author(s):  
M A Latif ◽  
A Lupi ◽  
D R G Schleicher ◽  
G D’Amico ◽  
P Panci ◽  
...  

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