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Related papers: Extra dimensions, SN1987a, and nucleon-nucleon sca…

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We show that in theories with large extra dimensions forces mediated by a bulk dilaton and bulk gauge fields may be parametrically (exponentially) weaker than gravity due to the suppression of their wave-functions on a brane. This is the…

High Energy Physics - Phenomenology · Physics 2009-10-31 Gia Dvali , Gregory Gabadadze , Massimo Porrati

A gravity-driven mechanism (``objective reduction'') proposed to explain quantum state reduction is analyzed in light of the possible existence of large extra dimensions in the ADD scenario. By calculating order-of-magnitude estimates for…

General Relativity and Quantum Cosmology · Physics 2008-11-26 J. R. Mureika

Resonant active-to-active ($\nu_a \to \nu_a$), as well as active-to-sterile ($\nu_a \to \nu_s$) neutrino ($\nu$) oscillations can take place during the core bounce of a supernova collapse. Besides, over this phase, weak magnetism increases…

Astrophysics · Physics 2009-08-07 Herman J. Mosquera Cuesta , Karen Fiuza

The aim of this talk is to provide non-experts with a brief and elementary introduction on the field of extra dimensions. The main motivation for extra dimensions relies on the more fundamental string theories that predict ten (or eleven)…

High Energy Physics - Phenomenology · Physics 2007-05-23 M. Quiros

We derive the graviton propagator on the brane for theories with quasi-localized gravity. In these models the ordinary 4D graviton is replaced by a resonance in the spectrum of massive Kaluza-Klein modes, which can decay into the extra…

High Energy Physics - Theory · Physics 2009-09-17 Csaba Csaki , Joshua Erlich , Timothy J. Hollowood

Despite their use as cosmological distance indicators and their importance in the chemical evolution of galaxies, the unequivocal identification of the progenitor systems and explosion mechanism of normal type Ia supernova (SN Ia) remains…

High Energy Astrophysical Phenomena · Physics 2017-05-15 Warren P. Wright , James P. Kneller , Sebastian T. Ohlmann , Friedrich K. Roepke , Kate Scholberg , Ivo R. Seitenzahl

The observation of neutrinos from Supernova~1987A has confirmed the theoretical conjecture that these particles play a crucial role during the collapse of the core of a massive star. Only one per cent of the energy they carry away from the…

Astrophysics · Physics 2007-05-23 H. -Th. Janka

In this note, we consider dijet production at gamma gamma colliders as a probe of recently proposed, large extra-dimensional gravity models. The exchange of virtual, spin-2 graviton towers (Kaluza-Klein excitations) significantly modifies…

High Energy Physics - Phenomenology · Physics 2008-11-26 M. A. Doncheski , R. W. Robinett

Neutrino emissions from electron/positron capture on the deuteron and the nucleon-nucleon fusion processes in the surface region of a supernova core are studied. These weak processes are evaluated in the standard nuclear physics approach,…

High Energy Astrophysical Phenomena · Physics 2015-06-18 S. Nasu , S. X. Nakamura , K. Sumiyoshi , T. Sato , F. Myhrer , K. Kubodera

The effects of classical gravitational radiation in models with large extra dimensions are investigated for ultra high energy cosmic rays (CRs). The cross sections are implemented into a simulation package (SENECA) for high energy hadron…

Astrophysics · Physics 2008-11-26 Ben Koch , Hans-Joachim Drescher , Marcus Bleicher

The diphoton excess around 750 GeV observed by ATLAS and CMS can be interpreted as coming from a massive spin-2 excitation. We explore this possibility in the context of warped five-dimensional models with the Standard Model (SM) fields…

High Energy Physics - Phenomenology · Physics 2016-07-13 Adam Falkowski , Jernej F. Kamenik

Neutrinos are guaranteed to be observable from the next galactic supernova (SN). Optical light and gravitational waves are also observable, but may be difficult to observe if the location of the SN in the galaxy or the details of the…

We show that the more energetic superluminal neutrinos with quadratically dispersed superluminalities \delta=\beta^2-1, for \beta=v/c where v is the neutrino velocity, also lose significant energy to radiation to the \nu+e^-+e^+ final state…

High Energy Physics - Phenomenology · Physics 2015-06-03 B. F. L. Ward

I calculate the diffuse flux of electron antineutrinos from all supernovae using the information on the neutrino spectrum from SN987A and the information on the rate of supernovae from direct supernova observations. The interval of flux…

Astrophysics · Physics 2009-11-13 Cecilia Lunardini

Small realistic Majorana neutrino masses can be generated via a Higgs triplet $(\xi^{++}, \xi^+, \xi^0)$ without having energy scales larger than $M_*={\cal O}(1)$ TeV in the theory. The large effective mass scale $\Lambda$ in the…

High Energy Physics - Phenomenology · Physics 2009-10-31 Ernest Ma , Martti Raidal , Utpal Sarkar

The exclusive gamma-met signal has a small standard model cross-section and is thus a good channel in which to look for signs of new physics. This signature is predicted by models with a superlight gravitino or with large extra spatial…

High Energy Physics - Experiment · Physics 2012-08-27 CDF Collaboration

We develop the theory of interaction of classical plasma with Kaluza-Klein (KK) gravitons in the ADD model of TeV-scale gravity. Plasma is described within the kinetic approach as the system of charged particles and Maxwell field both…

High Energy Physics - Phenomenology · Physics 2011-01-27 E. Yu. Melkumova

The idea of the magnetorotational explosion mechanism is that the energy of rotation of the neutron star formed in the course of a collapse is transformed into the energy of an expanding shock wave by means of a magnetic field. In the…

High Energy Astrophysical Phenomena · Physics 2019-04-01 G. S. Bisnovatyi-Kogan , S. G. Moiseenko , N. V. Ardelyan

Discovering neutrino decay would be strong evidence of physics beyond the Standard Model. Presently, there are only lax lower limits on the lifetime $\tau$ of neutrinos, of $\tau/m \sim 10^{-3}$ s eV$^{-1}$ or worse, where $m$ is the…

High Energy Astrophysical Phenomena · Physics 2020-04-16 Mauricio Bustamante

Light hypothetical particles with masses up to $\mathcal{O}(100)\ {\rm MeV}$ can be produced in the core of supernovae. Their subsequent decays to neutrinos can produce a flux component with higher energies than the standard flux. We study…

High Energy Physics - Phenomenology · Physics 2024-07-12 Kensuke Akita , Sang Hui Im , Mehedi Masud , Seokhoon Yun