arXiv:hep-th/0308055 v2 23 Sep 2003
elpolm ie h ag ag faalbeflxsadba and fluxes available of theory. range large We the satisfied. given are problem, energy real inflationary of stabilization, source volume the of and space, method mode the inflation about brane assumptions that tive conclude non-generi We the arise. discuss not We does inflation. problem for steep too furt mod it a typically renders reveals pactification moduli the string of closed stabilization the bran of of consideration difficulty ful well-known one evading potential, see geometry pactification warped a sight first At theory.
d
aaIsiueo udmna eerh oiBah od M Road, Bhabha Homi Research, Fundamental of Institute Tata
eivsiaeteebdigo rn nainit tbec stable into inflation brane of embedding the investigate We
******@,,******@. ******@, ******@, ******@st ******@, ******@,
a
eateto hsc,Safr nvriy tnod A9 CA Stanford, University, Stanford Physics, of Department
unMaldacena, Juan
o ad naini tigTheory String in Inflation Towards
c
b
nttt o dacdSuy rneo,N 84,USA 08540, NJ Princeton, Study, Advanced for Institute
LC tnodUiest,Safr,C 40,USA 94309, CA Stanford, University, Stanford SLAC,
hmtKachru, Shamit
c
imMcAllister, Liam
a,b
eaaKallosh, Renata
a
n adpP Trivedi P. Sandip and
a
in
nriLinde, Andrei
,
fisteifltnptniland potential inflaton the ifies
odtosudrwihthis which under conditions c
krudgoere nstring in geometries ckground
st rdc aual flat naturally a produce to ms
e btce superpotential obstacle: her
-- scenarios. e-antibrane
ru htti a o ea be not may this that argue
h apn fteinternal the of warping the
scnol oki restric- if work only can ls
matfiain fstring of ompactifications
ma 0 0,INDIA 005, 400 umbai
a
35 USA 4305,
TIFR/TH/03-06 SU-ITP-03/18 SLAC-PUB-9669 hep-th/0308055
d
1. Introduction
Inflation provides pelling explanation for the homogeneity and isotropy of
physics papers - andrei linde (2003), towards inflation in string theory 来自淘豆网m.daumloan.com转载请标明出处.