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相关论文: Extra dimensions, SN1987a, and nucleon-nucleon sca…

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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…

高能物理 - 唯象学 · 物理学 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…

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

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

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

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…

高能物理 - 唯象学 · 物理学 2011-04-11 V. H. Satheesh Kumar , P. K. Suresh , P. K. Das

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

The existence of compact dimensions which are accessible only to gravity represents an intriguing possible solution to the hierarchy problem. At present the strongest constraint on the existence of such compact Gravity-Only Dimensions…

天体物理学 · 物理学 2008-11-26 Christoph Hanhart , Jose A. Pons , Daniel R. Phillips , Sanjay Reddy

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…

高能物理 - 唯象学 · 物理学 2009-10-31 Schuyler Cullen , Maxim Perelstein

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

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

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

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

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…

核理论 · 物理学 2009-11-07 Daniel Arndt

We consider the production of gravitons via two photon fusion in Kaluza-Klein theories which allow TeV scale gravitational interactions. We find that the processes l+ l- to l+ l- + graviton, with l=electron or muon can put quite stringent…

高能物理 - 唯象学 · 物理学 2007-05-23 David Atwood , Shaouly Bar-Shalom , Amarjit Soni

We consider the production of gravitons via two photon and electron-photon fusion in Kaluza-Klein theories which allow TeV scale gravitational interactions. We show that at electron-positron colliders, the processes l+l- -> l+ l- graviton,…

高能物理 - 唯象学 · 物理学 2009-10-31 David Atwood , Shaouly Bar-Shalom , Amarjit Soni

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

Graviton production due to collapsing extra dimensions is studied. The momenta lying in the extra dimensions are taken into account. A $D$-dimensional background is matched to an effectively four-dimensional standard radiation dominated…

高能物理 - 唯象学 · 物理学 2009-11-07 Kerstin E. Kunze , Mairi Sakellariadou

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

We report on a search for large extra dimensions in a data sample of approximately 1 fb^{-1} of ppbar collisions at sqrt(s) = 1.96 TeV. We investigate Kaluza-Klein graviton production with a photon and missing transverse energy in the final…

高能物理 - 实验 · 物理学 2008-11-26 D0 Collaboration , V. M. Abazov
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