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Supernovae (SNe) are copious sources for Kaluza-Klein gravitons which are generic for theories with large extra dimensions. These massive particles are produced with average velocities ~0.5 c so that many of them are gravitationally…

高能物理 - 唯象学 · 物理学 2008-11-26 Steen Hannestad , Georg 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…

高能物理 - 唯象学 · 物理学 2011-05-05 Steen Hannestad , Georg Raffelt

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…

核理论 · 物理学 2014-11-18 Christoph Hanhart , Daniel R. Phillips , Sanjay Reddy , Martin J. Savage

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…

高能物理 - 唯象学 · 物理学 2009-02-23 Prasanta Kumar Das , V H Satheeshkumar , P. K. Suresh

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:…

高能物理 - 唯象学 · 物理学 2025-11-07 Edward Hardy , Anton Sokolov , Henry Stubbs

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…

高能物理 - 唯象学 · 物理学 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…

高能物理 - 唯象学 · 物理学 2008-11-26 Michel Casse , Jacques Paul , Gianfranco Bertone , Guenter Sigl

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…

高能物理 - 唯象学 · 物理学 2009-10-31 Ashok Goyal , Abhinav Gupta , Namit Mahajan

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…

高能物理 - 唯象学 · 物理学 2008-11-26 Jonathan L. Feng , Arvind Rajaraman , Fumihiro Takayama

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)…

天体物理学 · 物理学 2016-08-30 S. Cassisi , V. Castellani , S. Degl'Innocenti G. Fiorentini , B. Ricci

The constraint on the ADD model of extra dimensions coming from photon annihilation into Kaluza-Klein graviton in supernova cores is revisited. In the two photon process for a conservative choice of the core parameters, we obtain the bound…

天体物理学 · 物理学 2013-11-04 V. H. Satheeshkumar , P. K. Suresh

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…

高能物理 - 唯象学 · 物理学 2007-06-29 David Gherson

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.…

高能天体物理现象 · 物理学 2026-03-31 Georg G. Raffelt , Hans-Thomas Janka , Damiano F. G. Fiorillo

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…

高能物理 - 唯象学 · 物理学 2008-11-26 David Gherson

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…

高能物理 - 唯象学 · 物理学 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…

高能物理 - 唯象学 · 物理学 2024-10-08 David McKeen , John Ng , Michael Shamma

It is widely believe that galactic cosmic rays are originated in supernova remnants (SNRs) where they are accelerated by diffusive shock acceleration process at supernova blast waves driven by expanding SNRs. In recent theoretical…

高能天体物理现象 · 物理学 2017-08-02 Prabir Banik , Arunava Bhadra

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…

宇宙学与河外天体物理 · 物理学 2019-10-30 Michel Cassé , Bruno Mansoulié , Joseph Silk

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…

高能物理 - 唯象学 · 物理学 2009-11-07 Steen Hannestad

We investigate the theoretical and observational implications of the acceleration of protons and heavier nuclei in supernova remnants (SNRs). By adopting a semi-analytical technique, we study the non-linear interplay among particle…

高能天体物理现象 · 物理学 2017-08-23 D. Caprioli , P. Blasi , E. Amato
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