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Related papers: Pair Multiplicities and Pulsar Death

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Non-linear Compton scattering of ultra-relativistic electrons traversing high-intensity laser pulses generates also hard photons. These photon high-energy tails are considered for parameters in reach at the forthcoming experiments LUXE and…

High Energy Physics - Phenomenology · Physics 2021-03-10 B. Kampfer , A. I. Titov

The Compton process with the initial states of photons and neutrons described by the density matrices of a general form is studied for low energies of photons. The coherent contribution to the inclusive probability to record a photon is…

High Energy Physics - Phenomenology · Physics 2026-05-12 P. O. Kazinski , A. A. Sokolov

The radiation by relativistic plasma particles is beamed in the direction of field line tangents in the corotating frame, but in an inertial frame it is aberrated toward the direction of rotation. We have revised the relation of aberration…

Astrophysics · Physics 2007-05-23 R. T. Gangadhara

In the average profiles of several radio pulsars, the main pulse is accompanied by the preceding component. This so called precursor is known for its distinctive polarization, spectral, and fluctuation properties. Recent single-pulse…

Astrophysics · Physics 2009-11-13 S. A. Petrova

We consider the formation of RbCs by an elliptically polarized laser pulse. By varying the ellipticity of the laser for sufficiently large laser intensity, we see that the formation probability presents a strong dependence, especially…

Atomic Physics · Physics 2019-02-06 J. Pablo Salas , Cristel Chandre , J Salas

Pulse profiles of accreting millisecond pulsars can be used to determine neutron star (NS) parameters, such as their masses and radii, and therefore provide constraints on the equation of state of cold dense matter. Information obtained by…

High Energy Astrophysical Phenomena · Physics 2023-10-18 Anna Bobrikova , Vladislav Loktev , Tuomo Salmi , Juri Poutanen

The leading-particle effect and the factorization property of the scattering amplitude in the impact parameter space are used to study semiclassical production of pions in the central region. The mechanism is related to the isospin-uniform…

High Energy Physics - Phenomenology · Physics 2011-04-15 M. Martinis , V. Mikuta-Martinis , J. Črnugelj

The nature of coherent radio emission is still challenging even after more than half a century of pulsar discovery, but it is generally a consensus that single-pulse observations are essential for probing the magnetospheric dynamics,…

High Energy Astrophysical Phenomena · Physics 2026-05-11 Shunshun Cao , Yanjun Guo , Jinchen Jiang , Kejia Lee , Weiyang Wang , Renxin Xu

The importance of the photon-photon pair production process ($\gamma+ \gamma^{\prime}\to e^{+}+e^{-}$) to form pair production cascades in pulsar polar caps is investigated within the framework of the Ruderman-Sutherland vacuum gap model.…

Astrophysics · Physics 2007-05-23 Bing Zhang , G. J. Qiao

The complete absence of radio pulsars with periods exceeding a few seconds has lead to the popular notion of the existence of a high $P$ death line. In the standard picture, beyond this boundary, pulsars with low spin rates cannot…

Astrophysics · Physics 2009-10-30 Matthew G. Baring , Alice K. Harding

We discuss non-thermal emission mechanism of the Crab-like pulsars with both a two-dimensional electrodynamical study and a three-dimensional model. We investigate the emission process in the outer gap accelerator. In the two-dimensional…

Astrophysics · Physics 2009-11-13 J. Takata , H. -K. Chang

The aim of this work is to study the possible effects and biases on the radius constraints for rotation-powered millisecond pulsars when using Thomson approximation to describe electron scattering in the atmosphere models, instead of using…

High Energy Astrophysical Phenomena · Physics 2019-07-02 T. Salmi , V. Suleimanov , J. Poutanen

High-quality averaged radio profiles of some pulsars exhibit double, highly symmetric features both in emission and absorption. It is shown that both types of features are produced by a split-fan beam of extraordinary-mode curvature…

Solar and Stellar Astrophysics · Physics 2015-05-13 J. Dyks , B. Rudak , P. Demorest

The pion and quark annihilation mechanisms of dilepton production during relativistic nuclear collisions are studied. We focus on the modifications caused by the specific features of in-medium pion and quark states rather than by medium…

Nuclear Theory · Physics 2009-11-11 Dmitry Anchishkin

Models for the evolution of magnetic fields of neutron stars are constructed, assuming the field is embedded in the proton superconducting core of the star. The rate of expulsion of the magnetic flux out of the core, or equivalently the…

Astrophysics · Physics 2014-10-13 M. Jahan-Miri

The recent discovery of a population of eccentric (e ~ 0.1) millisecond pulsar (MSP) binaries with low-mass white dwarf companions in the Galactic field represents a challenge to evolutionary models that explain MSP formation as recycling:…

High Energy Astrophysical Phenomena · Physics 2016-12-21 E. D. Barr , P. C. C. Freire , M. Kramer , D. J. Champion , M. Berezina , C. G. Bassa , A. G. Lyne , B. W. Stappers

We study nonperturbative multiphoton electron-positron pair creation in ultrastrong electromagnetic fields formed by two counterpropagating pulses with elliptic polarization. Our numerical approach allows us to take into account the…

Atomic Physics · Physics 2015-06-25 Anton Wöllert , Heiko Bauke , Christoph H. Keitel

In the advent of next generation gamma-ray missions, we present general properties of spectral features of high-energy emission above $1\MeV$ expected for a class of millisecond, low magnetic field ($\sim 10^9\G$) pulsars. We extend…

Astrophysics · Physics 2009-10-31 T. Bulik , B. Rudak , J. Dyks

We report on the laser-driven generation of purely neutral, relativistic electron-positron pair plasmas. The overall charge neutrality, high average Lorentz factor ($\gamma_{e/p} \approx 15$), small divergence ($\theta_{e/p} \approx 10 -…

We consider stimulated pair production employing strong-field QED in a high-intensity laser background. In an infinite plane wave, we show that light-cone quasi-momentum can only be transferred to the created pair as a multiple of the laser…

High Energy Physics - Phenomenology · Physics 2010-08-23 Thomas Heinzl , Anton Ilderton , Mattias Marklund
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