Closed universes can satisfy the holographic principle in three dimensions
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[1] Cristián Martínez,et al. Cosmological scaling solutions of minimally coupled scalar fields in three dimensions , 2000, gr-qc/0007038.
[2] L. Susskind,et al. TASI lectures on the Holographic Principle , 2000, hep-th/0002044.
[3] Bin Wang,et al. Holography in (2+1)-dimensional cosmological models , 1999, hep-th/9910185.
[4] R. Wald,et al. Proof of classical versions of the Bousso entropy bound and of the generalized second law , 1999, hep-th/9908070.
[5] R. Bousso. A covariant entropy conjecture , 1999, hep-th/9905177.
[6] Andrei Linde,et al. Cosmology versus holography , 1999, hep-th/9904120.
[7] S. Rama. Holographic principle in the closed universe: a resolution with negative pressure matter , 1999, hep-th/9904110.
[8] G. Veneziano. Pre-bangian origin of our entropy and time arrow , 1999, hep-th/9902126.
[9] L. Susskind,et al. Holography and cosmology , 1998, hep-th/9806039.
[10] P. Steinhardt,et al. Resolving the cosmological missing energy problem , 1998, astro-ph/9804285.
[11] E. Witten. Anti-de Sitter space and holography , 1998, hep-th/9802150.
[12] A. Polyakov,et al. Gauge Theory Correlators from Non-Critical String Theory , 1998, hep-th/9802109.
[13] J. Maldacena. The Large-N Limit of Superconformal Field Theories and Supergravity , 1997, hep-th/9711200.
[14] P. Steinhardt,et al. Cosmological imprint of an energy component with general equation of state , 1997, astro-ph/9708069.
[15] M. Visser. General relativistic energy conditions: The Hubble expansion in the epoch of galaxy formation , 1997, gr-qc/9705070.
[16] L. Susskind,et al. M theory as a matrix model: A Conjecture , 1996, hep-th/9610043.
[17] J. Frieman,et al. Dynamical Lambda models of structure formation , 1996, astro-ph/9608122.
[18] L. Susskind. The world as a hologram , 1994, hep-th/9409089.
[19] G. Hooft. Dimensional Reduction in Quantum Gravity , 1993, gr-qc/9310026.
[20] J. Bekenstein,et al. Entropy bounds and black hole remnants. , 1993, Physical review. D, Particles and fields.
[21] P. Peebles,et al. Cosmological consequences of a rolling homogeneous scalar field. , 1988, Physical review. D, Particles and fields.
[22] J. Barrow,et al. Three-dimensional classical spacetimes , 1986 .
[23] J. Bekenstein. Entropy content and information flow in systems with limited energy , 1984 .
[24] S. Hawking. Breakdown of Predictability in Gravitational Collapse , 1976 .
[25] Matt Visser,et al. Lorentzian Wormholes: From Einstein to Hawking , 1995 .