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Related papers: MeV gamma rays from Q-ball decay

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Supersymmetric extensions of the Standard Model predict the existence of Q-balls with baryon and lepton numbers. Stable Q-balls can form at the end of inflation from the fragmentation of the Affleck-Dine condensate and can exist as dark…

High Energy Physics - Phenomenology · Physics 2007-05-23 Alexander Kusenko

We have shown that inflatons with a mass which is calculated to be of the order of $10^{10}\GeV$ can constitute a dominant part of dark matter. They can decay uniquely into a neutrino and antineutrino with a lifetime calculated to be…

Astrophysics · Physics 2007-05-23 Saul Barshay , Georg Kreyerhoff

The decay of dark matter particles which are coupled predominantly to charged leptons has been proposed as a possible origin of excess high-energy positrons and electrons observed by cosmic-ray telescopes PAMELA and Fermi LAT. Even though…

High Energy Physics - Phenomenology · Physics 2015-03-17 Mathias Garny , Alejandro Ibarra , David Tran , Christoph Weniger

A supersymmetric model with four generations is proposed, in which the top quark is approximately degenerate in mass with the $W^{\pm}$ gauge boson, $m_t\simeq m_W$, leading to values of $R_b$ in better agreement with the present…

High Energy Physics - Phenomenology · Physics 2008-11-26 M. Carena , H. E. Haber , C. E. M. Wagner

We calculate limits to the properties of massive, unstable neutrinos using data from gamma-ray detectors on the Pioneer Venus Orbiter Satellite; a massive neutrino emitted from SN1987A that decayed in flight and produced gamma rays would be…

Astrophysics · Physics 2008-11-26 A. Jaffe , M. S. Turner

We numerically study the formation of the gauge-mediation type Q balls in the logarithmic square potential on three-dimensional lattices. We obtain the broad charge distribution of the Q ball of this type for the first time. The charge of…

High Energy Physics - Phenomenology · Physics 2025-10-23 Shinta Kasuya , Masahiro Kawasaki

The widths of a glueball decay to two pions or kaons are analyzed in the pQCD framework. Our results show that the glueball ground state has small branching ratio for two-meson decay mode, which is around $10^{-2}$. The predicted values are…

High Energy Physics - Phenomenology · Physics 2009-10-30 Jun Cao , Tao Huang , Hui-fang Wu

We investigate the Q-ball decay in the gauge-mediated SUSY breaking. Q balls decay mainly into nucleons, and partially into gravitinos, while they are kinematically forbidden to decay into sparticles which would be cosmologically harmful.…

High Energy Physics - Phenomenology · Physics 2015-05-28 Shinta Kasuya , Masahiro Kawasaki

In theories with low energy supersymmetry breaking, the effective potential for squarks and sleptons has generically nearly flat directions, V(phi) ~ M^4 (log(phi/M))^n. This guarantees the existence of stable non-topological solitons,…

High Energy Physics - Phenomenology · Physics 2008-11-26 M. Laine , M. Shaposhnikov

The pi+pi- atom decays -in the ground state - predominantly into two neutral pions. We present a general expression for the corresponding decay width in the framework of QCD (including photons). It contains all terms at leading and…

High Energy Physics - Phenomenology · Physics 2009-10-31 A. Gall , J. Gasser , V. E. Lyubovitskij , A. Rusetsky

Radiative magnetic dipole decays of heavy-light vector mesons into pseudoscalar mesons V -> P\gamma are considered within the relativistic quark model. The light quark is treated completely relativistically, while for the heavy quark the…

High Energy Physics - Phenomenology · Physics 2009-11-07 D. Ebert , R. N. Faustov , V. O. Galkin

We obtain the spectrum of gamma ray emissions from the moduli whose decay into $e^+ e^-$ accounts for the 511 keV line observed by SPI/INTERGRAL. The moduli emit gamma rays through internal bremsstrahlung, and also decay directly into two…

Astrophysics · Physics 2009-11-11 Shinta Kasuya , Masahiro Kawasaki

We examine some general astrophysical results which can be related to the hypothesis that very heavy, metastable particles constitute compact, very massive central entities in QSO's and the core of galaxies. The mass and lifetime have been…

Astrophysics · Physics 2010-12-03 Saul Barshay , Georg Kreyerhoff

We consider different types of Q-balls as self-interacting dark matter. For the Q-balls to act as the dark matter of the universe they should not evaporate, which requires them to carry very large charges; depending on the type, the minimum…

High Energy Physics - Phenomenology · Physics 2009-11-07 K. Enqvist , A. Jokinen , T. Multamaki , I. Vilja

Since the era of the Fermi/LAT and atmospheric Cerenkov telescopes, pulsars are known to emit high and very high-energy photons, in the MeV-GeV range and sometimes up to TeV. To date, it is still unclear where and how these photons are…

High Energy Astrophysical Phenomena · Physics 2019-02-13 Jérôme Pétri

We have calculated the opacities and secondary production mechanisms of high energy photons arising in gamma-ray burst internal shocks, using exact cross-sections for the relevant processes. We find that for reasonable choices of…

Astrophysics · Physics 2010-11-15 Soebur Razzaque , Peter Meszaros , Bing Zhang

Usually the charge and the energy of stable Q-balls vary in a wide range or are even unbounded. In the present paper we study an interesting possibility that this range is parametrically small. In this case the spectra of stable Q-balls…

High Energy Physics - Theory · Physics 2014-07-07 E. Ya. Nugaev , M. N. Smolyakov

We study long-term evolution of radiating quasi-Q-balls in 1+1 dimensional models without mass threshold. Two different models are considered, the model with a rational modification of the usual Q-ball sextic potential and the model of a…

High Energy Physics - Theory · Physics 2025-03-12 Tomasz Romanczukiewicz , Yakov Shnir

Classical novae produce radioactive nuclei which are emitters of gamma-rays in the MeV range. Some examples are the lines at 478 and 1275 keV (from 7Be and 22Na) and the positron-electron annihilation emission, with the 511 keV line and a…

High Energy Astrophysical Phenomena · Physics 2013-05-06 M. Hernanz

The Galactic centre is a bright gamma-ray source with the GeV-TeV band spectrum composed of two distinct components in the 1-10 GeV and 1-10 TeV energy ranges. The nature of these two components is not clearly understood. We investigate the…

High Energy Astrophysical Phenomena · Physics 2015-09-30 D. Malyshev , M. Chernyakova , A. Neronov , R. Walter