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In theories with large extra dimensions, supernova (SN) cores are powerful sources of Kaluza-Klein (KK) gravitons. A large fraction of these massive particles are gravitationally retained by the newly born neutron star (NS). The subsequent…

High Energy Physics - Phenomenology · Physics 2025-04-03 S. Hannestad , G. G. Raffelt

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 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

An intriguing feature of extra dimensions is the possible production of Kaluza--Klein gravitons by nucleon-nucleon bremsstrahlung in the course of core collapse of massive stars, as pointed out by Hannestad and Raffelt. In this event…

High Energy Physics - Phenomenology · Physics 2008-11-26 Michel Casse , Jacques Paul , Gianfranco Bertone , Guenter Sigl

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

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

One of the strongest constraints on the existence of large, compact, "gravity-only" dimensions comes from SN1987a. If the rate of energy loss into these putative extra dimensions is too high, then the neutrino pulse from the supernova will…

Nuclear Theory · Physics 2014-11-18 Christoph Hanhart , Daniel R. Phillips , Sanjay Reddy , Martin J. Savage

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

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

In large extra dimensional Kaluza-Klein (KK) scenario, where the usual Standard Model (SM) matter is confined to a 3+1-dimensional hypersurface called the 3-brane and gravity can propagate to the bulk (D=4+d, d being the number of extra…

High Energy Physics - Phenomenology · Physics 2009-02-23 Prasanta Kumar Das , V H Satheeshkumar , P. K. Suresh

In models of universal extra dimensions, gravity and all standard model fields propagate in the extra dimensions. Previous studies of such models have concentrated on the Kaluza-Klein (KK) partners of standard model particles. Here we…

High Energy Physics - Phenomenology · Physics 2008-11-26 Jonathan L. Feng , Arvind Rajaraman , Fumihiro Takayama

We calculate the production of massive Kaluza-Klein(KK) modes via nucleon-nucleon gravi-bremsstrahlung in the early universe. Overproduction of these states would result in early matter domination and therefore a low age for the universe so…

High Energy Physics - Phenomenology · Physics 2008-11-26 Malcolm Fairbairn

The core of a massive star (M > 8 Msun) eventually collapses. This implosion usually triggers a supernova (SN) explosion that ejects most of the stellar envelope and leaves behind a neutron star (NS) with a mass of up to about 2 Msun.…

High Energy Astrophysical Phenomena · Physics 2026-03-31 Georg G. Raffelt , Hans-Thomas Janka , Damiano F. G. Fiorillo

Cosmic ray events above $10^{20}$ eV are on the verge of confronting fundamental particle physics. The neutrino is the only candidate primary among established particles capable of crossing 100 Mpc intergalactic distances unimpeded. The…

High Energy Physics - Phenomenology · Physics 2009-10-31 P. Jain , Douglas W. McKay , S. Panda , John P. Ralston

If the neutrinos are to be identified with the primary source of ultra-high energy cosmic rays(UHECR), their interaction on relic neutrinos is of great importance in understanding their long intergalactic journey. In theories with large…

High Energy Physics - Phenomenology · Physics 2009-10-31 Ashok Goyal , Abhinav Gupta , Namit Mahajan

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

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

Since the dawn of the new millennium, there has been a revived interest in the concept of extra dimensions.In this scenario all the standard model matter and gauge fields are confined to the 4 dimensions and only gravity can escape to…

High Energy Physics - Phenomenology · Physics 2011-04-11 V. H. Satheesh Kumar , P. K. Suresh , P. K. Das

The shape of the neutrino pulse from the supernova SN1987a provides one of the most stringent constraints on the size of large, compact, "gravity-only" extra dimensions. Previously, calculations have been carried out for a newly-born…

Nuclear Theory · Physics 2009-11-07 Daniel Arndt

We study the consequences of the gravitino decay into dark matter. We suppose that the lightest neutralino is the main component of dark matter. In our framework gravitino is heavy enough to decay before Big Bang Nucleosynthesis starts. We…

High Energy Physics - Phenomenology · Physics 2007-06-29 David Gherson
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