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相关论文: MeV gamma rays from Q-ball decay

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Mirror matter models have been suggested recently as an explanation of neutrino puzzles and microlensing anomalies. We show that mirror supernovae can be a copious source of energetic gamma rays if one assumes that the quantum gravity scale…

天体物理学 · 物理学 2011-05-23 R. N. Mohapatra , S. Nussinov , V. L. Teplitz

The sudden release of copious $\g$-ray photons into a compact region creates an opaque photon--lepton fireball due to the prolific production of electron--positron pairs. The photons that we observe in the bursts emerge only at the end of…

天体物理学 · 物理学 2007-05-23 Tsvi Piran

We study the decay properties of a heavy-light meson. We reformulate the decay amplitudes for the heavy-light systems and find a new way to calculate decay rates. Applying this formulation, we find a new sum rule for the radiative decays of…

高能物理 - 唯象学 · 物理学 2011-02-22 Takayuki Matsuki , Koichi Seo

We have calculated the width of the rare decay $H\to\gamma\gamma Z$ at one-loop level in the standard model for Higgs boson masses in the range $115 {\rm GeV} \leq m_H \leq 160 {\rm GeV}$ . For this range of Higgs boson masses we find that…

高能物理 - 唯象学 · 物理学 2009-11-10 Ali Abbasabadi , Wayne W. Repko

Gamma-ray photons from young pulsars allow the deepest insight into the properties and interactions of high-energy particles with magnetic and photon fields in a pulsar magnetosphere. Measurements with the Compton Gamma-Ray Observatory have…

天体物理学 · 物理学 2009-09-29 Gottfried Kanbach

Partial decay widths of the heavy-light mesons, $D, D_s, B,$ and $B_s$, emitting one chiral particle ($\pi$ or $K$) are evaluated in the framework of a relativistic potential model. Decay amplitudes are calculated by keeping the Lorentz…

高能物理 - 唯象学 · 物理学 2012-02-16 Takayuki Matsuki , Koichi Seo

It is argued that the quark mass difference $m_b-m_c$ can be extracted with a high accuracy from experimental data on ratia of moments of lepton energy spectrum in semileptonic decays of $B$ mesons. Theoretical expressions for the moments…

高能物理 - 唯象学 · 物理学 2011-01-25 Mikhail Voloshin

In a Pulsar Wind Nebula (PWN), the lifetime of inverse Compton emitting electrons exceeds the lifetime of its progenitor pulsar, but it exceeds also the age of the electrons that emit via synchrotron radiation; i.e. while the PWN grows…

高能天体物理现象 · 物理学 2015-05-30 O. Tibolla , K. Mannheim , S. Kaufmann , D. Elsässer

Excited Q-balls are studied by numerical simulations in the Minimal Supersymmetric Standard Model with supersymmetry broken by a gravity mediated mechanism. It is found that there is a suppression factor of $\cO(10^{-2})$ in the rate at…

高能物理 - 唯象学 · 物理学 2009-11-07 Tuomas Multamaki

The pion-bump structure in the gamma-ray spectrum is a direct proof for the hadronic origin of the gamma rays, and thus the decisive evidence for the acceleration of hadronic cosmic rays in astrophysical objects. However, the identification…

高能天体物理现象 · 物理学 2024-06-07 Jiahao Liu , Bing Liu , Ruizhi Yang

A theory is proposed to explain with simplicity the basic observed properties of a Gamma Ray Burst (GRB). It employs a well-known result of Schwinger, that static electric fields in excess of a critical value are unstable to pair creation,…

天体物理学 · 物理学 2007-05-23 R. Lieu , Y. Takahashi , T. W. B. Kibble

In a Pulsar Wind Nebula (PWN), the lifetime of inverse Compton emitting electrons exceeds the lifetime of its progenitor pulsar, but it exceeds also the age of the electrons that emit via synchrotron radiation; i.e. during the evolution of…

高能天体物理现象 · 物理学 2011-11-08 O. Tibolla , K. Mannheim , D. Elsässer , S. Kaufmann

We study Q-ball formation in the expanding universe on 1D, 2D and 3D lattice simulations. We obtain detailed Q-ball charge distributions, and find that the distribution is peaked at Q^{3D}_{peak} \simeq 1.9\times 10^{-2} (|\Phi_{in}|/m)^2,…

高能物理 - 唯象学 · 物理学 2014-11-20 Takashi Hiramatsu , Masahiro Kawasaki , Fuminobu Takahashi

The naturalness problem of PQ symmetry motivates study of the heavy QCD axion, with masses $m_a >$ 1 MeV generated at scales above the QCD scale, and low values of the PQ symmetry breaking scale, $f_a$. We compute the abundance of such…

高能物理 - 唯象学 · 物理学 2022-05-25 David I. Dunsky , Lawrence J. Hall , Keisuke Harigaya

We revisit the constraints implied by SN 1987 A observations on the decay rate of a multi-MeV $\nu_\tau$ decaying into the visible channel $\nu_\tau \rightarrow e^+ e^- \nu_e$, if its lifetime is more than 10 {\it sec.}. We discuss its…

高能物理 - 唯象学 · 物理学 2009-10-22 R. N. Mohapatra , S. Nussinov , X. Zhang

Gamma ray lines are expected to be emitted as part of the afterglow of supernova explosions, because radioactive decay of freshly synthesised nuclei occurs. Significant radioactive gamma ray line emission is expected from 56Ni and 44Ti…

高能天体物理现象 · 物理学 2017-10-25 Roland Diehl

We calculate two- and three-body decays of the (lightest) vector glueball into (pseudo)scalar, (axial-)vector, as well as pseudovector and excited vector mesons\textbf{ }in the framework of a model of QCD. While absolute values of widths…

高能物理 - 唯象学 · 物理学 2017-06-14 Francesco Giacosa , Julia Sammet , Stanislaus Janowski

The invariant mass spectrum of the lepton pair in inclusive semileptonic $\bar B\to X_u \ell\bar\nu$ decay yields a model independent determination of $|V_{ub}|$. Unlike the lepton energy and hadronic invariant mass spectra, nonperturbative…

高能物理 - 唯象学 · 物理学 2007-05-23 Christian W. Bauer , Zoltan Ligeti , Michael Luke

It is proposed that the gamma ray burst photons near the peak of the spectrum at several hundred KeV are produced on very compact scales, where photon production is limited by blackbody effects and/or the requirement of energetic quanta…

天体物理学 · 物理学 2009-10-31 D. Eichler , A. Levinson

Glueballs remain an experimentally undiscovered prediction of QCD. Lattice QCD predicts a spectrum of glueballs, with the tensor $(J^{PC}=2^{++})$ glueball being the second lightest, behind the scalar glueball. From an effective hadronic…

高能物理 - 唯象学 · 物理学 2023-10-18 Arthur Vereijken