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Particle physics model of inflation and the cosmological density perturbation
"... This is a review of models of inflation, and their predictions for the primordial curvature perturbation that is thought to be the origin of structure in the Universe. The spectral index n, specifying the scale-dependence of the spectrum of the curvature perturbation, will be a powerful discriminato ..."
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Cited by 163 (7 self)
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This is a review of models of inflation, and their predictions for the primordial curvature perturbation that is thought to be the origin of structure in the Universe. The spectral index n, specifying the scale-dependence of the spectrum of the curvature perturbation, will be a powerful discriminator between models, when it is measure with accuracy ∆n ∼ 0.01. The usual formula for n is derived, as well as its less familiar extension to the case of a multi-component inflaton; in both cases the key ingredient is the separate evolution of causally disconnected regions of the Universe. Primordial gravitational waves will be an even more powerful discriminator if they are observed, since most models of inflation predict that they are completely negligible. We focus on the new wave of models, which are firmly rooted in modern particle theory and have supersymmetry as a crucial ingredient. The essential particle theory background is summarized, first at an elementary level and later at a more advanced one. The review is addressed to both astrophysicists and particle physicists, and each section is fairly homogeneous regarding the assumed background knowledge.
The holographic principle
- Rev. Mod. Phys
, 2002
"... There is strong evidence that the area of any surface limits the information content of adjacent spacetime regions, at 1.4 ×10 69 bits per square meter. We review the developments that have led to the recognition of this entropy bound, placing special emphasis on the quantum properties of black hole ..."
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Cited by 132 (9 self)
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There is strong evidence that the area of any surface limits the information content of adjacent spacetime regions, at 1.4 ×10 69 bits per square meter. We review the developments that have led to the recognition of this entropy bound, placing special emphasis on the quantum properties of black holes. The construction of light-sheets, which associate relevant spacetime regions to any
Electroweak baryon number nonconservation in the early universe and in highenergy collisions,”Uspekhi
- Fizicheskikh Nauk,
, 1996
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The pre-big bang scenario in string cosmology
- Phys. Rept
, 2003
"... We review physical motivations, phenomenological consequences, and open problems of the so-called pre-big bang scenario in superstring cosmology. Contents 1 ..."
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Cited by 89 (3 self)
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We review physical motivations, phenomenological consequences, and open problems of the so-called pre-big bang scenario in superstring cosmology. Contents 1
Towards inflation in string theory
- JCAP
, 2003
"... We investigate the embedding of brane inflation into stable compactifications of string theory. At first sight a warped compactification geometry seems to produce a naturally flat inflaton potential, evading one well-known difficulty of brane-antibrane scenarios. Careful consideration of the closed ..."
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Cited by 82 (9 self)
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We investigate the embedding of brane inflation into stable compactifications of string theory. At first sight a warped compactification geometry seems to produce a naturally flat inflaton potential, evading one well-known difficulty of brane-antibrane scenarios. Careful consideration of the closed string moduli reveals a further obstacle: superpotential stabilization of the compactification volume typically modifies the inflaton potential and renders it too steep for inflation. We discuss the non-generic conditions under which this problem does not arise. We conclude that brane inflation models can only work if restrictive assumptions about the method of volume stabilization, the warping of the internal space, and the source of inflationary energy are satisfied. We argue that this may not be a real problem, given the large range of available fluxes and background geometries in string theory.
Metric-affine f(R) theories of gravity
- J. Suppl. Ser
, 2007
"... Modified gravity theories have received increased attention lately due to combined motivation coming from high-energy physics, cosmology and astrophysics. Among numerous alternatives to Einstein’s theory of gravity, theories which include higher order curvature invariants, and specifically the parti ..."
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Cited by 69 (1 self)
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Modified gravity theories have received increased attention lately due to combined motivation coming from high-energy physics, cosmology and astrophysics. Among numerous alternatives to Einstein’s theory of gravity, theories which include higher order curvature invariants, and specifically the particular class of f(R) theories, have a long history. In the last five years there has
Computational capacity of the universe
- Physical Review Letters
"... Merely by existing, all physical systems register information. And by evolving dynamically in time, they transform and process that information. The laws of physics determine the amount of information that a physical system can register (number of bits) and the number of elementary logic operations ..."
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Cited by 55 (0 self)
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Merely by existing, all physical systems register information. And by evolving dynamically in time, they transform and process that information. The laws of physics determine the amount of information that a physical system can register (number of bits) and the number of elementary logic operations that a system can perform (number of ops). The universe is a physical system. This paper quantifies the amount of information that the universe can register and the number of elementary operations that it can have performed over its history. The universe can have performed no more than 10 120 ops on 10 90 bits. ‘Information is physical ’ 1. This statement of Landauer has two complementary interpretations. First, information is registered and processed by physical systems. Second, all physical systems register and process information. The description of physical systems in terms of information and information processing is complementary to the conventional description of physical system in terms of the laws of physics. A recent paper by the author2 put bounds on the amount of information processing that can be performed by physical systems. The first limit is on speed. The Margolus/Levitin theorem3 implies that the total
The Cosmological Constant and the String Landscape
"... Theories of the cosmological constant fall into two classes, those in which the vacuum energy is fixed by the fundamental theory and those in which it is adjustable in some way. For each class we discuss key challenges. The string theory landscape is an example of an adjustment mechanism. We discuss ..."
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Cited by 49 (1 self)
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Theories of the cosmological constant fall into two classes, those in which the vacuum energy is fixed by the fundamental theory and those in which it is adjustable in some way. For each class we discuss key challenges. The string theory landscape is an example of an adjustment mechanism. We discuss the status of this idea, and future directions. Rapporteur talk at the 23rd Solvay Conference in Physics, December, 2005. 1 The cosmological constant I would like to start by drawing a parallel to an earlier meeting — not a Solvay conference, but the 1947 Shelter Island conference. In both cases a constant of nature was at the center of discussions. In each case theory gave an unreasonably large or infinite value for the constant, which had therefore been assumed to vanish for reasons not yet understood, but in each case experiment or observation had recently found a nonzero value. At Shelter
Large Scale Structure And Supersymmetric Inflation Without Fine Tuning,” Phys
- Rev. Lett
, 1994
"... We explore constraints on the spectral index n of density fluctuations and the neutrino energy density fraction ΩHDM, employing data from a variety of large scale observations. The best fits occur for n ≈ 1 and ΩHDM ≈ 0.15 − 0.30, over a range of Hubble constants 40 − 60 km s −1 Mpc −1. We present a ..."
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Cited by 48 (0 self)
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We explore constraints on the spectral index n of density fluctuations and the neutrino energy density fraction ΩHDM, employing data from a variety of large scale observations. The best fits occur for n ≈ 1 and ΩHDM ≈ 0.15 − 0.30, over a range of Hubble constants 40 − 60 km s −1 Mpc −1. We present a new class of inflationary models based on realistic supersymmetric grand unified theories which do not have the usual ‘fine tuning ’ problems. The amplitude of primordial density fluctuations, in particular, is found to be proportional to (MX/MP) 2, where MX(MP) denote the GUT (Planck) scale, which is reminiscent of cosmic strings! The spectral index n = 0.98, in excellent agreement with the observations provided the dark matter is a mixture of ‘cold’ and ‘hot ’ components. PACS Nos: 98.80Cq, 98.65Dx, 12.10Dm, 11.30Pb 1 Recent studies of large scale structure formation [1], when confronted with
