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Related papers: Low-energy Gravitino Interactions

200 papers

Low-energy tests of fundamental symmetries and studies of neutrino properties provide a powerful window on physics beyond the Standard Model (BSM). In this article, we provide a basic theoretical framework for a subsequent set of articles…

High Energy Physics - Phenomenology · Physics 2015-06-15 Vincenzo Cirigliano , Michael J. Ramsey-Musolf

We show that the nonlinear supersymmetric effective lagrangian can be used for model-independent parameterization of the light gravitino scattering amplitude at energies up to and above the soft supersymmetry-breaking masses. This provides…

High Energy Physics - Phenomenology · Physics 2014-11-17 Taekoon Lee , Guo-Hong Wu

We discuss $\nu - \gamma$ interactions in the presence of a homogeneous magnetic field with energies less than pair production threshold. The neutrinos are taken to be massless with only standard-model couplings. The magnetic field fulfills…

High Energy Physics - Phenomenology · Physics 2007-05-23 A. Ioannisian

Low-energy nuclear weak-interaction processes play important roles in many astrophysical contexts, and effective field theory is believed to be a highly useful framework for describing these processes in a model-independent manner. I…

Nuclear Theory · Physics 2007-05-23 K. Kubodera

An overview of neutrino electromagnetic properties, which open a door to the new physics beyond the Standard Model, is given. The effects of neutrino electromagnetic interactions both in terrestrial experiments and in astrophysical…

High Energy Physics - Phenomenology · Physics 2016-04-20 Carlo Giunti , Konstantin A. Kouzakov , Yu-Feng Li , Alexey V. Lokhov , Alexander I. Studenikin , Shun Zhou

Electron energy and angular distributions in the process of low-energy elastic neutrino-electron scattering are treated in the free-electron approximation. The effects of the millicharges, magnetic, electric, and anapole moments of massive…

High Energy Physics - Phenomenology · Physics 2017-11-03 Konstantin A. Kouzakov , Alexander I. Studenikin

I review the constraints on the mass of gravitinos that follow from considerations on energy loss in stars and from Big Bang Nucleosynthesis arguments.

High Energy Physics - Phenomenology · Physics 2009-10-31 J. A. Grifols

Using the effective Lagrangian for the low energy photon-photon interaction the lowest order photon self energy at finite temperature and in non-equilibrium is calculated within the real time formalism. The Debye mass, the dispersion…

High Energy Physics - Phenomenology · Physics 2009-10-31 Markus H. Thoma

We generalize the low-energy theorems of gluodynamics to finite temperature. Examples of the theorems in the low and high temperature limits are given.

Nuclear Theory · Physics 2009-10-31 P. J. Ellis , J. I Kapusta , H. -B. Tang

We discuss the concept and design of effective atom-atom potentials that accurately describe any physical processes involving only states around the threshold. The existence of such potentials gives hope to a quantitative, and systematic,…

Atomic Physics · Physics 2009-11-07 Bo Gao

The low energy effective field theory of interacting neutrinos derived from the Standard Model may be framed as a pointlike interaction and thereby modeled on a lattice of neutrino momenta. We identify a path to take a continuum limit of…

High Energy Physics - Phenomenology · Physics 2026-02-09 Michael J. Cervia

The mechanism of low energy physics formation in the framework of multidimensional gravity is discussed. It is shown that a wide set of parameters of a primary theory could lead to the observable Universe. Quantum fluctuations of extra…

General Relativity and Quantum Cosmology · Physics 2013-02-12 S. G. Rubin

We consider a many particle quantum system, in which each particle interacts only with its nearest neighbours. Provided that the energy per particle has an upper bound, we show, that the energy distribution of almost every product state…

Mathematical Physics · Physics 2009-11-10 M. Hartmann , G. Mahler , O. Hess

We briefly review the high energy astrophysical processes that are related to the production of high energy $\gamma$-ray and neutrino signals and are likely to be important for the energy loss of high and ultrahigh energy cosmic rays. We…

Astrophysics · Physics 2007-05-23 Todor Stanev

Dyson (2013) argued that the extraordinarily large number of gravitons in a gravitational wave makes them impossible to be resolved as individual particles. While true, it is shown in this paper that a LIGO interferometric detector also…

High Energy Astrophysical Phenomena · Physics 2018-10-17 Richard Lieu

Low energy neutrino processes are ideal probes for new Physics beyond the Standard Model. Cosmological observations and rare nuclear processes can test neutrino mass scales and give definite answers to unsolved basic questions like the…

High Energy Physics - Phenomenology · Physics 2008-11-26 Oliviero Cremonesi , Alessandro Melchiorri

The least action principle played a central role in the development of modern physics. A major drawback of the principle is that its applicability is limited to holonomic constraints. In the present work, we investigate the energy lost by…

Classical Physics · Physics 2025-02-14 C. Ortiz , R. S. Khatiwada

I review basic concepts in the nonequilibrium physics of small systems, emphasizing single molecule experiments and how they contribute to expanding our current understanding of energy and information.

Biological Physics · Physics 2024-04-09 Felix Ritort

Observables in few-nucleon scattering processes are sensitive probes to study the two and many-body interactions between nucleons in nuclei. In the past decades, several facilities provided a large data base to study in detail the…

Nuclear Experiment · Physics 2010-02-09 Johan Messchendorp

The interactions of gravitons with matter are calculated in parallel with the familiar photon case. It is shown that graviton scattering amplitudes can be factorized into a product of familiar electromagnetic forms, and cross sections for…

General Relativity and Quantum Cosmology · Physics 2009-11-11 Barry R. Holstein