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相关论文: Dark energy and the hierarchy problem

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We revisit the case of scalar dark matter interacting just gravitationally with the Standard Model (SM) particles in an extra-dimensional Randall-Sundrum scenario. We assume that both, the dark matter and the Standard Model, are localized…

高能物理 - 唯象学 · 物理学 2020-02-06 Miguel G. Folgado , Andrea Donini , Nuria Rius

Apart from its gravitational interactions, dark matter (DM) has remained so far elusive in laboratory searches. One possible explanation is that the relevant interactions to explain its relic abundance are mainly gravitational. In this work…

高能物理 - 唯象学 · 物理学 2026-01-12 Andrea Donini , Miguel G. Folgado , Juan Herrero-García , Giacomo Landini , Alejandro Muñoz-Ovalle , Nuria Rius

If low-energy supersymmetry is the solution to the hierarchy problem, it is a puzzle why supersymmetric particles have not been observed experimentally to date. We show that supersymmetric particles in the TeV region can be explained if the…

高能物理 - 唯象学 · 物理学 2011-04-18 Fuminobu Takahashi , Tsutomu T. Yanagida

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

At high energies on a cosmological brane of Randall-Sundrum type, particle interactions can produce gravitons that are emitted into the bulk and that can feed a bulk black hole. We generalize previous investigations of such radiating…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Laszlo Gergely , Emily Leeper , Roy Maartens

We propose an extended version of the standard model, in which neutrino oscillation, dark matter, and baryon asymmetry of the Universe can be simultaneously explained by the TeV-scale physics without assuming unnatural hierarchy among the…

高能物理 - 唯象学 · 物理学 2009-02-27 Mayumi Aoki , Shinya Kanemura , Osamu Seto

Explanations of the late-time cosmic acceleration within the framework of general relativity are plagued by difficulties. General relativistic models are mostly based on a dark energy field with fine-tuned, unnatural properties. There is a…

天体物理学 · 物理学 2010-04-22 Ruth Durrer , Roy Maartens

In looking for imprints of extra dimensions in brane world models one usually builts these so that they are compatible with known low energy physics and thus focuses on high energy effects. Nevertheless, just as submillimeter Newton's law…

高能物理 - 唯象学 · 物理学 2008-11-26 Roman Linares , Hugo A. Morales-Tecotl , Omar Pedraza

In the context of a toy model we discuss the phenomenon of colliding five-branes, with two of the extra space dimensions compactified on tori. In one of the branes (hidden world) the torus is magnetised. Assuming opposite-tension branes, we…

高能物理 - 理论 · 物理学 2014-11-18 Elias Gravanis , Nick E. Mavromatos

We consider Randall-Sundrum model with localized gravity, replacing the extra compact space-like dimension by a time-like one. In this way the solution to the hierarchy problem can be reconciled with a correct cosmological expansion of the…

高能物理 - 理论 · 物理学 2009-10-31 Masud Chaichian , Archil B. Kobakhidze

We discuss and compare the effects of one extra dimension in the Randall Sundrum models on the evaluation of the Casimir force between two parallel plates. We impose the condition that the result reproduce the experimental measurements…

高能物理 - 唯象学 · 物理学 2008-11-26 Mariana Frank , Ismail Turan , Lorric Ziegler

A braneworld model for neutrino Dark Energy (DE) is presented. We consider a five dimensional two-branes set up with a bulk scalar field motivated by supergravity. Its low-energy effective theory is derived with a moduli space approximation…

高能物理 - 唯象学 · 物理学 2009-09-29 Andrea Zanzi

We discuss a TeV scale model which would explain neutrino oscillation, dark matter, and baryon asymmetry of the Universe simultaneously by the dynamics of the extended Higgs sector and TeV-scale right-handed neutrinos with imposed an exact…

高能物理 - 唯象学 · 物理学 2009-05-26 Mayumi Aoki , Shinya Kanemura , Osamu Seto

We regard the Casimir energy of the universe as the main contribution to the cosmological constant. Using 5 dimensional models of the universe, the flat model and the warped one, we calculate Casimir energy. Introducing the new…

高能物理 - 理论 · 物理学 2015-06-05 Shoichi Ichinose

We consider the cosmology and hierarchy of scales in models with branes immersed in a five-dimensional curved spacetime subject to radion stabilization. The universe naturally find itself in the radiation-dominated epoch when the…

高能物理 - 唯象学 · 物理学 2009-10-31 Danny Marfatia

It has been suggested that the dark energy density \rho_v ~ 10^{-12} eV^4 in the universe is associated with a metastable (false) vacuum, while the true vacuum has a vanishing cosmological constant. By including supergravity corrections we…

高能物理 - 唯象学 · 物理学 2009-11-11 Qaisar Shafi , Arunansu Sil , Siew-Phang Ng

A very simple mechanism is proposed that stabilizes the orbifold geometry within the context of the Randall-Sundrum proposal for solving the hierarchy problem. The electroweak TeV scale is generated from the Planck scale by spontaneous…

高能物理 - 理论 · 物理学 2007-05-23 Israel Quiros

The fact that the energy densities of dark energy and matter are similar currently, known as the coincidence problem, is one of the main unsolved problems of cosmology. We present here a model in which a spatial curvature of the universe…

天体物理学 · 物理学 2009-11-13 Urbano Franca

The hierarchy problem between the electroweak (EW) and Planck scales remains a central puzzle in modern physics. We discuss a promising solution operating through the cosmological selection of the EW vacuum in a multiverse landscape, where…

高能物理 - 唯象学 · 物理学 2026-05-28 Jin-Lei Yang , Frank F. Deppisch

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