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相关论文: Casimir-Induced Quintessence in Dark Dimension

200 篇论文

There exist field theory models where the fermionic energy-momentum tensor contains a term proportional to g_{\mu\nu}\bar{\Psi}\Psi which can be responsible for a dark matter to dark energy transmutation. We study some cosmological aspects…

高能物理 - 理论 · 物理学 2007-05-23 E. I. Guendelman , A. B. Kaganovich

Dynamical dark energy (DE) phenomenon emerges as a geometrical effect accompanying the cosmological expansion of nonrelativistic fermionic matter. This occurs without the need for any fluid, like e.g. dynamical scalar field (quintessence,…

广义相对论与量子宇宙学 · 物理学 2013-03-14 E. I. Guendelman , A. B. Kaganovich

We examine the lowest order quantum corrections to the effective action arising from a quantized real scalar field in the Randall-Sundrum background spacetime. The leading term is the familiar vacuum, or Casimir, energy density. The next…

高能物理 - 理论 · 物理学 2009-11-07 A. Flachi , D. J. Toms

We show that shape moduli in sub-millimeter extra dimensional scenarios, addressing the gauge hierarchy problem, can dominate the energy density of the universe today. In our scenario, the volume of the extra dimensions is stabilized at a…

高能物理 - 唯象学 · 物理学 2009-11-10 Marco Peloso , Erich Poppitz

An oscillating scalar field as a quintessence model for dark energy is proposed. The case of a power-law potential is particularly intriguing and is the focus of the present article. In this model the equation of state w_{OQ} of dark energy…

天体物理学 · 物理学 2007-11-26 Je-an Gu

We show that the chameleon scalar field can drive the current phase of cosmic acceleration for a large class of scalar potentials that are also consistent with local tests of gravity. These provide explicit realizations of a quintessence…

天体物理学 · 物理学 2008-11-26 Philippe Brax , Carsten van de Bruck , Anne-Christine Davis , Justin Khoury , Amanda Weltman

Unknown short-distance effects cancel the quartic divergence of the zero-point energies. If this renormalization took effect in the early universe after the last phase transition and applied only to modes whose wavelengths (over 2 pi) were…

高能物理 - 唯象学 · 物理学 2011-03-28 Kevin Cahill

A six parameter cosmological model, involving a vacuum energy density that is extremely tiny compared to fundamental particle physics scales, describes a large body of increasingly accurate astronomical data. In a first part of this brief…

高能物理 - 唯象学 · 物理学 2009-11-11 Norbert Straumann

We consider a cosmological solution which can explain anisotropic evolution of spatial dimensions and the stabilization of extra dimensions in brane gas formalism. We evaluate the effective potentials, induced by brane gas, bulk flux and…

高能物理 - 理论 · 物理学 2009-02-20 Jin Young Kim

We study the landscape of lower-dimensional vacua of the SM coupled to gravity in the presence of the ``dark dimension'' of size $R_\perp$ in the micron range, focusing on the validity of the swampland conjecture forbidding the presence of…

高能物理 - 唯象学 · 物理学 2024-01-10 Luis A. Anchordoqui , Ignatios Antoniadis , Jules Cunat

We derive a general formalism for constructing a four-dimensional effective action for the radion field in 5 dimensions, taking into account the possible dependence of the scale factor on the internal coordinate. First and second variations…

高能物理 - 唯象学 · 物理学 2008-11-26 Panagiota Kanti , Keith A. Olive , Maxim Pospelov

Cosmology enters precision testing period with the observational experiments advancement. We have not arrived to decipher the origin of the dominant dark energy component of our universe, although we have located some of its characters. In…

高能物理 - 唯象学 · 物理学 2007-05-23 Tomohiro Inagaki , Xinhe Meng , Tsukasa Murata

Recently, the self-tuning mechanism of cancellation of vacuum energy has been proposed in which our universe is a flat 3-brane in a 5-dimensional spacetime. In this letter, the self-tuning mechanism of dark energy is proposed by considering…

高能物理 - 理论 · 物理学 2009-10-31 K. Uzawa , J. Soda

The mystery of the Dark energy is not just its smallness. The extreme fine tuning of its density in the Early Universe such that it permits galaxy formation before creating a new inflationary epoch is its other unexplained aspect. Here we…

天体物理学 · 物理学 2007-05-23 Houri Ziaeepour

The well-known hierarchy between the Planck scale (~10^{19}GeV) and the TeV scale, namely a ratio of ~10^{16} between the two, is coincidentally repeated in a inverted order between the TeV scale and the dark energy scale at \~10^{-3}eV…

高能物理 - 唯象学 · 物理学 2009-08-03 Pisin Chen

We present updated constraints on an interacting dark energy - dark matter model with pure momentum transfer, where dark energy is in the form of a quintessence scalar field with an exponential potential. We run a suite of MCMC analyses…

宇宙学与河外天体物理 · 物理学 2026-02-09 Alkistis Pourtsidou

We compute the expectations of the squares of the electric and magnetic fields in the vacuum region outside a half-space filled with a uniform dispersive dielectric. We find a positive energy density of the electromagnetic field which…

量子物理 · 物理学 2009-11-07 V. Sopova , L. H. Ford

We study the role of the brane-induced graviton kinetic term in theories with large extra dimensions. In five dimensions we construct a model with a TeV-scale fundamental Planck mass and a {\it flat} extra dimension the size of which can be…

高能物理 - 唯象学 · 物理学 2008-11-26 Gia Dvali , Gregory Gabadadze , Marko Kolanovic , Francesco Nitti

We explore quintessence models of dark energy which exhibit non-minimal coupling between the dark matter and the dark energy components of the cosmic fluid. The kind of coupling chosen is inspired in scalar-tensor theories of gravity. We…

天体物理学 · 物理学 2007-05-23 Tame Gonzalez , Genly Leon , Israel Quiros

We show that the neutrino mass, the dark matter and the dark energy can be explained in a unified framework, postulating a new invisible Born-Infeld field, which we name "non-linear dark photon", undergoing a meV-scale dynamical…

高能物理 - 唯象学 · 物理学 2022-08-09 Andrea Addazi , Salvatore Capozziello , Qingyu Gan , Antonino Marcianò