scholarly journals The Dark-Matter Density Profiles and Binary Black Holes

2011 ◽  
Author(s):  
Li-Chin YEH
2010 ◽  
Vol 514 ◽  
pp. A47 ◽  
Author(s):  
S. Pasetto ◽  
E. K. Grebel ◽  
P. Berczik ◽  
R. Spurzem ◽  
W. Dehnen

2016 ◽  
Vol 456 (4) ◽  
pp. 3542-3552 ◽  
Author(s):  
Edouard Tollet ◽  
Andrea V. Macciò ◽  
Aaron A. Dutton ◽  
Greg S. Stinson ◽  
Liang Wang ◽  
...  

2007 ◽  
Vol 16 (07) ◽  
pp. 1243-1248 ◽  
Author(s):  
I. B. KHRIPLOVICH ◽  
N. PRODUIT

If primordial black holes (PBH) saturate the present upper limit on the dark matter density in our Solar system and if their radiation spectrum is discrete, the sensitivity of modern detectors is close to that necessary for detecting this radiation. This conclusion is not in conflict with the upper limits on the PBH evaporation rate.


2004 ◽  
Vol 352 (4) ◽  
pp. 1109-1120 ◽  
Author(s):  
Y. Ascasibar ◽  
G. Yepes ◽  
S. Gottlöber ◽  
V. Müller

2020 ◽  
Vol 904 (1) ◽  
pp. 45 ◽  
Author(s):  
Kohei Hayashi ◽  
Masashi Chiba ◽  
Tomoaki Ishiyama

2006 ◽  
Vol 453 (1) ◽  
pp. 21-25 ◽  
Author(s):  
T. Kronberger ◽  
M. P. Leubner ◽  
E. van Kampen

2010 ◽  
Vol 19 (11) ◽  
pp. 1873-1873
Author(s):  
ANTONINO DEL POPOLO ◽  
ISMAIL SAFFET YEŞILYURT

2014 ◽  
Vol 23 (1) ◽  
Author(s):  
A. Del Popolo

AbstractWe study through a semi-analytic model how the inner slopes of relaxed ΛCDM dark matter halos with and without baryons depend on the halo mass. We find that the inner logarithmic density slope, α ≡


Sign in / Sign up

Export Citation Format

Share Document