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Related papers: Cosmological Constraints on Large Extra Dimensions

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The existing cosmological constraints on theories with large extra dimensions rely on the thermal production of the Kaluza-Klein modes of gravitons and radions in the early Universe. Successful inflation and reheating, as well as…

High Energy Physics - Phenomenology · Physics 2011-10-11 Rouzbeh Allahverdi , Chris Bird , Stefan Groot Nibbelink , Maxim Pospelov

We have studied cosmological constraints on the number and radii of possible large extra dimensions. If such dimensions exist, Kaluza-Klein (KK) modes are copiously produced at high temperatures in the early universe, and can potentially…

High Energy Physics - Phenomenology · Physics 2009-11-07 Steen Hannestad

In the Kaluza-Klein (KK) scenario with n large extra dimensions where gravity propagates in the 4+n dimensional bulk of spacetime while gauge and matter fields are confined to a four dimensional subspace, the light graviton KK modes can be…

High Energy Physics - Phenomenology · Physics 2009-09-15 V. Barger , T. Han , C. Kao , R. -J. Zhang

We reconsider cosmological constraints on extra dimension theories from the excess production of Kaluza-Klein gravitons. We point out that, if the normalcy temperature is above 1 GeV, then graviton states produced at this temperature will…

High Energy Physics - Phenomenology · Physics 2009-11-10 Cosmin Macesanu , Mark Trodden

We derive the maximum fraction of energy emitted in the form of massive (Kaluza- Klein) gravitons by core collapse supernovae, and the corresponding minimal extra-dimensional Planck mass M* in the ADD gravity framework at TeV scales. Our…

Cosmology and Nongalactic Astrophysics · Physics 2019-10-30 Michel Cassé , Bruno Mansoulié , Joseph Silk

If large extra dimensions exist in nature, supernova (SN) cores will emit large fluxes of Kaluza-Klein gravitons, producing a cosmic background of these particles with energies and masses up to about 100 MeV. Radiative decays then give rise…

High Energy Physics - Phenomenology · Physics 2011-05-05 Steen Hannestad , Georg Raffelt

In theories with large extra dimensions, constraints from cosmology lead to non-trivial lower bounds on the fundamental scale M_F, corresponding to upper bounds on the radii of the compact extra dimensions. These constraints are especially…

High Energy Physics - Phenomenology · Physics 2008-11-26 Lawrence J. Hall , David Smith

We revisit cooling bounds on light Kaluza-Klein (KK) gravitons, as arise in the dark dimension scenario, considering red giants, neutron stars, and supernovae. In addition to bremsstrahlung, we account for two novel production channels:…

High Energy Physics - Phenomenology · Physics 2025-11-07 Edward Hardy , Anton Sokolov , Henry Stubbs

Cosmic super-strings interact generically with a tower of light and/or strongly coupled Kaluza-Klein (KK) modes associated with the geometry of the internal space. We study the production of KK particles by cosmic super-string loops, and…

High Energy Physics - Theory · Physics 2012-07-20 Jean-Francois Dufaux

Astrophysical constraints of new physics are often limited to weakly interacting light particles, such as axions, the Kaluza-Klein (KK) gravitons from the ADD model, sterile neutrinos and unparticles. We discuss the possibility for an…

High Energy Physics - Phenomenology · Physics 2008-08-09 Cong-Xin Qiu

We discuss in detail the information on large extra dimensions which can be derived in the framework of stellar evolution theory and observation. The main effect of large extra dimensions arises from the production of the Kaluza-Klein (KK)…

Astrophysics · Physics 2016-08-30 S. Cassisi , V. Castellani , S. Degl'Innocenti G. Fiorentini , B. Ricci

Two extra dimensions of micron scale might simultaneously address the gauge and cosmological hierarchy problems. In our paper we examine various observational bounds in scenarios with one and two large extra dimensions, to see if they are…

High Energy Physics - Theory · Physics 2025-07-28 Luis Anchordoqui , Ignatios Antoniadis , Dieter Lust

We present arguments that show why it is difficult to see \emph{rich} extra dimensions in the Universe. More precisely, we study the conditions under which significant size and variation of the extra dimensions in a Kaluza-Klein…

High Energy Physics - Theory · Physics 2022-01-26 Aghil Alaee , Marcus Khuri , Hari Kunduri

In models featuring extra spatial dimensions, particle collisions in the early universe can produce Kaluza-Klein gravitons. Such particles will later decay, potentially impacting the process of Big Bang nucleosynthesis. In this paper, we…

High Energy Physics - Phenomenology · Physics 2024-07-11 Mathieu Gross , Dan Hooper

Neutrino masses and quantum gravity are strong reasons to extend the standard model of particle physics. A large extra dimension can be motivated by quantum gravity and can explain the small neutrino masses with new singlet states that…

High Energy Physics - Phenomenology · Physics 2024-10-08 David McKeen , John Ng , Michael Shamma

We use experimental limits on Lorentz violation to obtain new constraints on Kaluza-Klein-type theories in which the extra dimensions may be large but do not necessarily have units of length. The associated variation in fundamental…

High Energy Physics - Phenomenology · Physics 2016-07-18 James M. Overduin , Hamna Ali

In this paper, the generation of topological energy in models with large extra dimensions is investigated. The origin of this energy is attributed to a topological deformation of the standard Minkowski vacuum due to compactification of…

High Energy Physics - Theory · Physics 2007-05-23 Abhinav Gupta

Recent models invoking extra spacelike dimensions inhabited by (bulk) neutrinos are shown to have significant cosmological effects if the size of the largest extra dimension is R > 1 fm. We consider effects on cosmic microwave background…

High Energy Physics - Phenomenology · Physics 2009-10-31 Kevork Abazajian , George M. Fuller , Mitesh Patel

The lightest Kaluza-Klein particle appearing in models with universal extra dimensions has recently been proposed as a viable dark matter candidate when the extra dimensions are compactified on a scale of the order of 1 TeV. Underlying…

Astrophysics · Physics 2009-11-07 Torsten Bringmann , Martin Eriksson , Michael Gustafsson

Recently there has been a lot of interest in models in which gravity becomes strong at the TeV scale. The observed weakness of gravitational interactions is then explained by the existence of extra compact dimensions of space, which are…

High Energy Physics - Phenomenology · Physics 2009-10-31 Schuyler Cullen , Maxim Perelstein
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