CAN GALACTIC HALOS BE MADE OF AXIONS

被引:190
作者
IPSER, J
SIKIVIE, P
机构
关键词
D O I
10.1103/PhysRevLett.50.925
中图分类号
O4 [物理学];
学科分类号
0702 ;
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页码:925 / 927
页数:3
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[1]  
ABBOT L, UNPUB
[2]  
BARR S, 1982, 4004822P2 U WASH REP
[3]  
BARR S, 1982, 4004818P2 U WASH REP
[4]  
BOND JR, 1980, PHYS REV LETT, V45, P1980, DOI 10.1103/PhysRevLett.45.1980
[5]   UPPER LIMIT ON NEUTRINO REST MASS [J].
COWSIK, R ;
MCCLELLAND, J .
PHYSICAL REVIEW LETTERS, 1972, 29 (10) :669-+
[6]   THE FORMATION OF GALAXIES FROM MASSIVE NEUTRINOS [J].
DAVIS, M ;
LECAR, M ;
PRYOR, C ;
WITTEN, E .
ASTROPHYSICAL JOURNAL, 1981, 250 (02) :423-431
[7]   ASTROPHYSICAL BOUNDS ON VERY-LOW-MASS AXIONS [J].
DICUS, DA ;
KOLB, EW ;
TEPLITZ, VL ;
WAGONER, RV .
PHYSICAL REVIEW D, 1980, 22 (04) :839-845
[8]  
DIMOPOULOS S, 1982, HUTP82A040 HARV U RE
[9]   A SIMPLE SOLUTION TO THE STRONG CP PROBLEM WITH A HARMLESS AXION [J].
DINE, M ;
FISCHLER, W ;
SREDNICKI, M .
PHYSICS LETTERS B, 1981, 104 (03) :199-202
[10]   DYNAMIC EVIDENCE ON MASSIVE CORONAS OF GALAXIES [J].
EINASTO, J ;
KAASIK, A ;
SAAR, E .
NATURE, 1974, 250 (5464) :309-310