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The Standard Model of particle physics and the theory of General Relativity (GR) currently provide a good description of almost all phenomena of particle physics and gravitation that have received controlled experimental tests. However, the…

原子物理 · 物理学 2009-01-23 Thomas Dent

I describe our understanding of physics near the planck length, in particular the great progress of the last four years in string theory. Superstring theory, and a recent extension called M theory, are leading candidates for a quantum…

高能物理 - 理论 · 物理学 2007-05-23 Joseph Kouneiher

This article aims at discussing the cosmological constant problem at a pedagogical but fully technical level. We review how the vacuum energy can be regularized in flat and curved space-time and how it can be understood in terms of Feynman…

宇宙学与河外天体物理 · 物理学 2015-06-05 Jerome Martin

In spite of its great phenomenological success, current models of scalar field-driven inflation suffer from important unresolved conceptual issues. New fundamental physics will be required to address these questions. String theory is a…

高能物理 - 理论 · 物理学 2008-11-26 Robert H. Brandenberger

Our current best guess for a unified theory of gravitation and quantum field theory (string theory) generically predicts a set of requirements for a consistently quantized theory, the Swampland criteria. Refined versions of these criteria…

宇宙学与河外天体物理 · 物理学 2023-08-09 Nils Schöneberg , Léo Vacher , J. D. F. Dias , Martim M. C. D. Carvalho , C. J. A. P. Martins

The old cosmological-constant (CC) problem indicates an inconsistency of the usual formulation of semiclassical gravity. The usual formulation of semiclassical gravity also seems to be inconsistent with the conventional interpretation of…

广义相对论与量子宇宙学 · 物理学 2007-05-23 H. Nikolic

This is an essay sketching the line of thinking which has led the present author to propose the constituent or atomic model of gravitation more than a decade ago. It turns out that viewing the problem of gravitation as a quantum many body…

天体物理学 · 物理学 2009-10-19 Pawel O. Mazur

We connect a possible solution for the ``cosmological constant problem'' to the existence of a (postulated) conformal fixed point in a fundamental theory. The resulting cosmology leads to quintessence, where the present acceleration of the…

高能物理 - 理论 · 物理学 2009-11-07 C. Wetterich

Unimodular gravity addresses the old cosmological constant (CC) problem, explaining why such constant is not at least as large as the largest particle mass scale, but classically it is indistinguishable from ordinary gravity. Conversely,…

高能物理 - 理论 · 物理学 2024-08-05 Alberto Salvio

In this article the cosmological constant problems, as well as the astronomical evidence for a cosmologically significant homogeneous exotic energy density with negative pressure (quintessence), are reviewed for a broad audience of…

天体物理学 · 物理学 2007-05-23 Norbert Straumann

The existence of a small, non-zero cosmological constant is one of the major puzzles in fundamental physics. Naively, quantum field theory arguments would imply a cosmological constant which is up to 10$^{120}$ times larger than the…

综合物理 · 物理学 2022-09-08 Michael Bishop , Joey Contreras , Peter Martin , Douglas Singleton

String theory axions appear to be promising candidates for explaining cosmological constant via quintessence. In this paper, we study conditions on the string compactifications under which axion quintessence can happen. For sufficiently…

高能物理 - 理论 · 物理学 2007-05-23 Peter Svrcek

Recent cosmological observations suggest the existence of a positive cosmological constant $\Lambda$ with the magnitude $\Lambda(G\hbar/c^3) \approx 10^{-123}$. This review discusses several aspects of the cosmological constant both from…

高能物理 - 理论 · 物理学 2008-11-26 T. Padmanabhan

Cosmic strings are linear concentrations of energy that form whenever phase transitions in the early universe break axial symmetries as originally shown by Kibble. They are the result of frustrated order in the quantum fields responsible…

天体物理学 · 物理学 2008-11-11 A. Achucarro , C. J. A. P. Martins

The idea that the vacuum energy density $\rho_{\Lambda}$ could be time dependent is a most reasonable one in the expanding Universe; in fact, much more reasonable than just a rigid cosmological constant for the entire cosmic history. Being…

广义相对论与量子宇宙学 · 物理学 2015-07-08 Harald Fritzsch , Joan Sola

There are two important examples of physical systems which violate the strong energy condition : Universes (like, it would seem, our own) with a positive cosmological constant, and wormholes. We suggest that a positive cosmological constant…

高能物理 - 理论 · 物理学 2008-11-26 Brett McInnes

A review is given on the consistency checks of GUT, which unify the electroweak and strong nuclear forces into a single theory. Such theories predict a new kind of force, which could provide answers to several open questions in cosmology.…

高能物理 - 唯象学 · 物理学 2010-01-22 W. de Boer

It is argued that classical string solutions should not be fine tuned to have a positive cosmological constant (CC) at the observed size, since even the quantum corrections from standard model effects will completely negate any classical…

高能物理 - 理论 · 物理学 2008-11-26 S. P. de Alwis

In discussing the construction of a consistent theory of quantum gravity unified with the gauge interactions we are naturally led to a string theory. We review its properties and the five consistent supersymmetric string theories in ten…

高能物理 - 理论 · 物理学 2009-10-30 Paolo Di Vecchia

Astronomical observations have shown that the expansion of the universe is at present accelerating, in a way consistent with the presence of a positive cosmological constant. This is a major puzzle, because we do not understand: why the…

天体物理学 · 物理学 2007-05-23 Jordi Miralda-Escude