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Related papers: Photon Pickup by Intense Poynting Flows

200 papers

We study the dependence of the electromagnetic luminosity --produced by interactions of force-free magnetospheres-- on dipole inclinations in binary neutron star systems. We show that this interaction extracts kinetic energy from the system…

General Relativity and Quantum Cosmology · Physics 2014-08-06 Marcelo Ponce , Carlos Palenzuela , Luis Lehner , Steven L. Liebling

We demonstrate that Kerr nonlinearity in optical circuits can lead to both resonant four-wave mixing and photon blockade, which can be used for high-yield generation of high-fidelity individual photon pairs with conjugated frequencies. We…

Quantum Physics · Physics 2018-05-21 Y. Sherkunov , D. M. Whittaker , V. Falko

The production of charged pion pairs via multiphoton absorption from an intense X-ray laser wave colliding with an ultrarelativistic proton beam is studied. Our calculations include the contributions from both the electromagnetic and…

High Energy Physics - Phenomenology · Physics 2011-02-15 Anis Dadi , Carsten Müller

Emission from X-ray binaries in the hard spectral state is dominated by high-energy radiation attributed to the Compton scattering of seed photons. The prevalent model of the Comptonization by hot electrons or pairs faces the problem of…

High Energy Astrophysical Phenomena · Physics 2026-05-26 John Groger , Kun Hu , Henric Krawczynski

In the Poynting Flux dominated outflow (the initial ratio of the electromagnetic energy flux to the particle energy flux $\sigma_0\gg1$) model for Gamma-ray bursts, nearly half of the internally dissipated magnetic energy is converted into…

Astrophysics · Physics 2007-05-23 Y. Z. Fan , D. M. Wei , C. F. Wang

The INTEGRAL satellite has revealed a major population of supergiant High Mass X-ray Binaries in our Galaxy, revolutionizing our understanding of binary systems and their evolution. This population, constituted of a compact object orbiting…

High Energy Astrophysical Phenomena · Physics 2010-05-13 Sylvain Chaty

Fast rotating cool stars are characterised by high magnetic activity levels and frequently show dark spots up to polar latitudes. Their distinctive surface distributions of magnetic flux are investigated in the context of the solar-stellar…

Astrophysics · Physics 2008-11-26 V. Holzwarth

We calculate the photon pair production rate in strong magnetic field created in off-central heavy-ion collisions. Photon decay leads to depletion of the photon yield by a few percent at RHIC and by as much as 20% at the LHC. It also…

Nuclear Theory · Physics 2011-02-21 Kirill Tuchin

Usually, photons are described by plane waves with a definite 4-momentum. In addition to plane-wave photons, "twisted photons" have recently entered the field of modern laser optics; these are coherent superpositions of plane waves with a…

Accelerator Physics · Physics 2016-06-24 U. D. Jentschura , V. G. Serbo

Highly luminous rapid flares are characteristic of processes around compact objects like white dwarfs, neutron stars or black holes. In the high energy regime of X- and gamma-rays, outbursts with variability time-scales of seconds and…

Astrophysics · Physics 2009-07-09 A. Stefanescu , G. Kanbach , A. Słowikowska , J. Greiner , S. McBreen , G. Sala

We use holographic methods to show that photons emitted by a strongly coupled plasma subject to a magnetic field are linearly polarized regardless of their four-momentum, except when they propagate along the field direction. The…

High Energy Physics - Theory · Physics 2025-11-17 Daniel Ávila , Tonantzin Monroy , Francisco Nettel , Leonardo Patiño

The existence of hot, two-temperature accretion flows is essential to the recent discussions of the low luminosity, hard X-ray emission from accreting neutron stars and black holes in Galactic binaries and massive black holes in low…

Astrophysics · Physics 2009-10-31 Jongmann Yang , Insu Yi

Line resolved X-ray spectra of outflows from X-ray binaries are interesting since they provide quantifiable measures of the accreted material on to the compact object (black hole or neutron star), which can not be observed directly in the…

High Energy Astrophysical Phenomena · Physics 2025-06-25 Noa Keshet , Ehud Behar , Jon M. Miller

The European gamma-ray observatory INTEGRAL has found a group of hard X-ray sources which are highly absorbed, i.e., with column densities higher than about 10^{23}/cm^2. Here I give an overview of this class of INTEGRAL sources. The X-ray,…

Astrophysics · Physics 2009-11-11 Erik Kuulkers

X-ray signatures of outflowing gas have been detected in several accreting black-hole binaries, always in the soft state. A key question raised by these observations is whether these winds might also exist in the hard state. Here, we carry…

The process of photon splitting $\gamma \to \gamma \gamma$ in a strong magnetic field is investigated both below and above the pair creation threshold. Contrary to the statement by Baier et al., the ``allowed'' channel $\alw$ is shown not…

High Energy Physics - Phenomenology · Physics 2009-10-31 M. V. Chistyakov , A. V. Kuznetsov , N. V. Mikheev

Production of a massive neutrino-antineutrino pair by a virtual polarized photon in the Weiberg-Salam model with mixing is studied. The rate of the neutrino production by photons with various polarizations is found at values of the magnetic…

High Energy Physics - Phenomenology · Physics 2007-05-23 V. Ch. Zhukovskii , A. E. Grigoruk , K. G. Levtchenko , P. A. Eminov

High velocity outflows from supermassive black holes have been invoked to explain the recent identification of strong absorption features in the hard X-ray spectra of several quasars. Here, Monte Carlo radiative transfer calculations are…

Astrophysics · Physics 2009-11-10 S. A. Sim

The common tunneling picture of electron-positron pair creation in a strong electric field is generalized to pair creation in combined crossed electric and magnetic fields. This enhanced picture, being symmetric for electrons and positrons,…

Quantum Physics · Physics 2015-03-20 Anton Wöllert , Michael Klaiber , Heiko Bauke , Christoph H. Keitel

If ultra-high energy cosmic rays (UHECRs) are accelerated at astrophysical point sources, the identification of such sources can be achieved if there is some kind of radiation at observable wavelengths that may be associated with the…

Astrophysics · Physics 2009-11-10 C. Ferrigno , P. Blasi , D. De Marco