Inflation from tachyon condensation, large N effects -: art. no. 103504

被引:39
作者
Majumdar, M
Davis, AC
机构
[1] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Theoret Phys Grp, London SW7 2BW, England
[2] Univ Cambridge, Ctr Math Sci, Dept Appl Math & Theoret Phys, Cambridge CB3 0WA, England
来源
PHYSICAL REVIEW D | 2004年 / 69卷 / 10期
关键词
D O I
10.1103/PhysRevD.69.103504
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Using only general properties of the tachyon potential we show that inflation may be generic when many branes and antibranes become coincident. Inflation may occur (1) because of the assistance of the many diagonal tachyon fields, (2) when the tachyons condense in a staggered fashion, or (3) when some of them condense very late. We point out that such inflation is in some sense a stringy implementation of chaotic inflation and may have important applications for "regularizing" a lopsided or singular cosmological compact surface.
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页数:8
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共 60 条
[1]   String thermodynamics in D-brane backgrounds [J].
Abel, SA ;
Barbón, JLF ;
Kogan, II ;
Rabinovici, E .
JOURNAL OF HIGH ENERGY PHYSICS, 1999, (04) :XXV-53
[2]  
ADAMS A, 2000, J HIGH ENERGY PHYS, P29
[3]  
[Anonymous], J HIGH ENERGY PHYS
[4]  
Bento MC, 2003, PHYS REV D, V67, DOI [10.1103/PhysRevD.67.063511, 10.1103/PhysRevD.67.023504]
[5]   On the cosmological relevance of the tachyon [J].
Choudhury, D ;
Ghoshal, D ;
Jatkar, DP ;
Panda, S .
PHYSICS LETTERS B, 2002, 544 (3-4) :231-238
[6]  
Cline JM, 2002, J HIGH ENERGY PHYS
[7]  
Danielsson U. H., 2001, J HIGH ENERGY PHYS, V09, P011
[8]  
Douglas MR, 2002, J HIGH ENERGY PHYS
[9]   Cosmological string gas on orbifolds [J].
Easther, R ;
Greene, BR ;
Jackson, MG .
PHYSICAL REVIEW D, 2002, 66 (02)
[10]  
EN A, 2002, J HIGH ENERGY PHYS, P3