Quick Search:
Prog. Theor. Phys. Supplement No.148 (2002) pp. 158-164
Cosmological Horizons, Quintessence and String Theory
Nemanja Kaloper*
Department of Physics, Stanford University, Stanford, CA 94305, USA
(Received August 15, 2002)
Abstract:
String theory is presently the best candidate for
a quantum theory of gravity unified with other forces.
It is natural to hope that applications of string theory to
cosmology may shed new light on the cosmological conundra,
such as singularities, initial conditions, cosmological constant
problem and the origin of inflation. Before we can apply string theory to
cosmology, there are important conceptual and practical problems
which must be addressed.
We have reviewed here some of these problems, related to
how one defines string theory in a cosmological setting.
URL :
http://ptp.ipap.jp/link?PTPS/148/158/
DOI : 10.1143/PTPS.148.158
References:
-
T. Banks, W. Fischler and L. Motl, J. High Energy Phys. 01 (1999), 019[IoP STACKS].
-
S. Perlmutter et al., Astrophys. J. 483 (1997), 565[CrossRef].
A. G. Riess et al., Astron. J. 116 (1998), 1009.
P. M. Garnavich et al., Astrophys. J. 509 (1998), 74[IoP STACKS].
S. Perlmutter et al., Astrophys. J. 517 (1999), 565[CrossRef].
-
T. Banks, hep-th/0007146[e-print arXiv];
hep-th/0011255[e-print arXiv].
T. Banks and W. Fischler, hep-th/0102077[e-print arXiv].
-
S. Hellerman, N. Kaloper and L. Susskind, J. High Energy Phys. 06 (2001), 003[IoP STACKS].
-
W. Fischler, A. Kashani-Poor, R. McNees and S. Paban, J. High Energy Phys. 07 (2001), 003[IoP STACKS].
-
E. Witten, hep-th/0106109[e-print arXiv].
- J. Maldacena and C. Nunez, Int. J. Mod. Phys. A 16 (2001), 822.
-
B. Ratra and P. J. E. Peebles, Phys. Rev. D 37 (1988), 3406[APS].
-
R. R. Caldwell, R. Dave and P. J. Steinhardt, Phys. Rev. Lett. 80 (1998), 1582[APS].
L. Wang, R. R. Caldwell, J. P. Ostriker and P. J. Steinhardt, Astrophys. J. 530 (2000), 17[CrossRef].
- S. W. Hawking and G. F. R. Ellis, The Large Scale Structure of Space-Time (Cambridge Univ. Press, Cambridge, 1972).
-
P. Breitenlohner and D. Z. Freedman, Phys. Lett. B 115 (1982), 197[CrossRef];
Ann. of Phys. 144 (1982), 249[CrossRef].
-
P. K. Townsend, Phys. Lett. B 148 (1984), 55[CrossRef].
K. Skenderis and P. K. Townsend, Phys. Lett. B 468 (1999), 46[CrossRef].
-
L. Dyson, M. Kleban and L. Susskind, J. High Energy Phys. 10 (2002), 011[IoP STACKS].
-
R. Kallosh, A. Linde, S. Prokushkin and M. Shmakova, hep-th/0208156[e-print arXiv].
-
C. Csaki, N. Kaloper and J. Terning, Phys. Rev. Lett. 88 (2002), 161302[APS];
Phys. Lett. B 535 (2002), 33[CrossRef].