Galaxy formation with cosmic strings and massive neutrinos

1988 ◽  
Vol 328 ◽  
pp. 23 ◽  
Author(s):  
Edmund Bertschinger ◽  
Paul N. Watts
1987 ◽  
Vol 78 (6) ◽  
pp. 1219-1224 ◽  
Author(s):  
Mizuo Izawa ◽  
Humitaka Sato

1988 ◽  
Vol 130 ◽  
pp. 560-561
Author(s):  
Robert H. Brandenberger

Hot dark matter particles have large thermal velocities at teg and hence cannot be gravitationally bound on small scales (free streaming). In models of formation of structure based on linear adiabatic perturbations all inhomogeneities on scales smaller than the maximal free streaming length λj are washed out. The mass λj inside a bail of radius exceeds the galaxy mass. Hence in the above models galaxies can only lorm by fragmentation of larger-scale objects. This is a severe problem.


1986 ◽  
Vol 75 (6) ◽  
pp. 1342-1350 ◽  
Author(s):  
H. Sato

1981 ◽  
Vol 245 ◽  
pp. L97 ◽  
Author(s):  
F. R. Klinkhamer ◽  
C. A. Norman

1989 ◽  
Vol 571 (1 Texas Symposi) ◽  
pp. 151-169 ◽  
Author(s):  
EDMUND BERTSCHINGER

Sign in / Sign up

Export Citation Format

Share Document