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The emissivity for the neutrino pair synchrotron radiation in strong magnetic fields has been calculated both analytically and numerically for high densities and moderate temperatures, as can be found in neutron stars. Under these…

Astrophysics · Physics 2009-10-28 A. Vidaurre , A. Perez , H. Sivak , J. Bernabeu , J. M. Ibanez

Light emission in the first hours and days following core-collapse supernovae (SNe) is dominated by the escape of photons from the expanding shock heated envelope. In a preceding paper, Paper I, we provided a simple analytic description of…

High Energy Astrophysical Phenomena · Physics 2024-02-05 Jonathan Morag , Ido Irani , Nir Sapir , Eli Waxman

We study the scattering theory for charged Klein-Gordon equations: \[\{{array}{l} (\p_{t}- \i v(x))^{2}\phi(t,x) \epsilon^{2}(x, D_{x})\phi(t,x)=0,[2mm] \phi(0, x)= f_{0}, [2mm] \i^{-1} \p_{t}\phi(0, x)= f_{1}, {array}. \] where:…

Mathematical Physics · Physics 2015-05-27 Christian Gérard

Unique optical properties of semiconductor nanoparticles (SN) make them very promising in the multitude of applications including lasing, light emission and photovoltaics. In many of these applications it is imperative to understand the…

Mesoscale and Nanoscale Physics · Physics 2017-01-04 Kirill A. Velizhanin

The frequency distribution of photons in frequency that results from single Compton scattering of monochromatic radiation on thermal electrons is derived in the mildly relativistic limit. Algebraic expressions are given for (1) the photon…

Astrophysics · Physics 2009-10-31 S. Y. Sazonov , R. A. Sunyaev

The observed spectrum of a supernova remnant (SNR) is a superposition of many ``local'' spectra emitted by regions of SNRs that are under different physical conditions. The question remains as to whether the broadening of the high-energy…

Astrophysics · Physics 2007-05-23 O. Petruk

In the standard synchrotron afterglow model, a power law of electrons is responsible for all aspects of photon production and absorption. Recent numerical work has shown that the vast majority of particles in the downstream medium are…

High Energy Astrophysical Phenomena · Physics 2018-08-22 Donald C. Warren , Maxim V. Barkov , Hirotaka Ito , Shigehiro Nagataki , Tanmoy Laskar

We present results from the Suzaku observation of the microquasar GRS 1915+105 performed during the 2005 October multiwavelength campaign. The data include both stable state (class \chi) and limit-cycle oscillation (class \theta). Correct…

High Energy Astrophysical Phenomena · Physics 2015-05-18 Y. Ueda , K. Honda , H. Takahashi , C. Done , H. Shirai , Y. Fukazawa , K. Yamaoka , S. Naik , H. Awaki , K. Ebisawa , J. Rodriguez , S. Chaty

We present ~400ks NuSTAR observations of the northeast (NE) and southwest (SW) non-thermal limbs of the Galactic SNR SN1006. We discovered three sources with X-ray emission detected at >50keV. Two of them are identified as background AGN.…

High Energy Astrophysical Phenomena · Physics 2018-09-19 Jiang-Tao Li , Jean Ballet , Marco Miceli , Ping Zhou , Jacco Vink , Yang Chen , Fabio Acero , Anne Decourchelle , Joel N. Bregman

Within an isospin- and momentum-dependent transport model for nuclear reactions at intermediate energies, we investigate the interplay of the nucleon-nucleon short-range correlations (SRC) and nuclear symmetry energy $E_{sym}(\rho)$ on hard…

Nuclear Theory · Physics 2018-01-08 Gao-Chan Yong , Bao-An Li

We consider the effect of electron scattering on lines emitted as a result of supernova interaction with a circumstellar medium, assuming that the scattering occurs in ionized gas in the preshock circumstellar medium. The single scattering…

High Energy Astrophysical Phenomena · Physics 2018-02-07 Chenliang Huang , Roger Chevalier

We present a theoretical study of Compton scattering of X- and $\gamma$-rays by a $K$-shell electron. Special attention is paid to the double-differential cross section and polarization of the scattered photons for linearly polarized…

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…

High Energy Physics - Phenomenology · Physics 2025-04-03 S. Hannestad , G. G. Raffelt

The scattering of kinks and low-frequency breathers of the nonlinear sine-Gordon (SG) equation on a spatially localized $\mathcal{PT}$-symmetric perturbation (defect) with a balanced gain and loss is investigated numerically. It is…

Pattern Formation and Solitons · Physics 2014-11-06 Danial Saadatmand , Sergey V. Dmitriev , Denis I. Borisov , P. G. Kevrekidis

Detailed information on the physical parameters in the sources of cosmological Gamma-Ray Bursts (GRBs) is obtained from few plausible assumptions consistent with observations. Model-independent requirements posed by these assumptions on the…

Astrophysics · Physics 2009-10-31 E. V. Derishev , V. V. Kocharovsky , Vl. V. Kocharovsky

The radiative loss interpretation for the broken power-law spectra of blazars is often questioned since the difference between the indices does not support this inference. Using the blazar Mkn 421 as a case study, we performed a detailed…

High Energy Astrophysical Phenomena · Physics 2022-06-22 C. Baheeja , S. Sahayanathan , Frank M. Rieger , Sitha K Jagan , C. D. Ravikumar

Context: The relation between Galactic cosmic-ray electrons, magnetic fields and synchrotron radiation. Aims: We exploit synchrotron radiation to constrain the low-energy interstellar electron spectrum, using various radio surveys and…

High Energy Astrophysical Phenomena · Physics 2011-10-03 A. W. Strong , E. Orlando , T. R. Jaffe

The one-dimensional Klein-Gordon equation is investigated with the most general Lorentz structure for the external potentials. The analysis and calculation of the reflection and transmission coefficients for the scattering of particles in a…

Quantum Physics · Physics 2008-11-26 Tatiana R. Cardoso , Antonio S. de Castro

Gamma-ray bursts (GRBs), among the most compelling astrophysical phenomena, are potential candidates for exploring the evolution of energy distribution among magnetic fields and particles through multiwavelength observations. The fraction…

High Energy Astrophysical Phenomena · Physics 2025-12-18 Nissim Fraija , Boris Betancourt-Kamenetskaia , Antonio Galván , Maria Dainotti

We demonstrate that the exact solution for the spectrum of synchrotron radiation from an isotropic population of mono-energetic electrons in turbulent magnetic field with Gaussian distribution of local field strengths can be expressed in…

High Energy Astrophysical Phenomena · Physics 2020-03-02 Evgeny Derishev , Felix Aharonian
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