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Related papers: Photon Pickup by Intense Poynting Flows

200 papers

Photosynthesis is a plausible pathway for the sustenance of a substantial biosphere on an exoplanet. In fact, it is also anticipated to create distinctive biosignatures detectable by next-generation telescopes. In this work, we explore the…

Earth and Planetary Astrophysics · Physics 2023-06-08 Manasvi Lingam , Amedeo Balbi , Swadesh M. Mahajan

X-ray absorption and emission lines now serve as powerful diagnostics of the outflows from active galaxies. Detailed X-ray line studies of outflows have recently been enabled for a significant number of active galaxies via the grating…

Astrophysics · Physics 2009-11-07 W. N. Brandt , S. Kaspi

We have estimated fluxes of neutrinos and gamma-rays that are generated from decays of charged and neutral pions from a pulsar surrounded by supernova ejecta in our galaxy, including an effect that has not been taken into consideration,…

Astrophysics · Physics 2009-11-10 S. Nagataki

The hard X-ray twisted photons and relativistic massive particles with orbital angular momentum -- vortex electrons, muons, protons, etc. -- have many potential applications in high-energy and nuclear physics. However, such states can be…

High Energy Physics - Phenomenology · Physics 2022-11-11 D. V. Karlovets , S. S. Baturin , G. Geloni , G. K. Sizykh , V. G. Serbo

On December 27, 2004, plasma particle detectors on the GEOTAIL spacecraft detected an extremely strong signal of hard X-ray photons from the giant flare of SGR1806-20, a magnetar candidate. While practically all gamma-ray detectors on any…

High mass accretion rate onto strongly magnetised neutron stars results in the appearance of accretion columns supported by the radiation pressure and confined by the strong magnetic field of a star. At mass accretion rates above $\sim…

High Energy Astrophysical Phenomena · Physics 2023-04-26 Aman Asthana , Alexander A. Mushtukov , Alexandra A. Dobrynina , Igor S. Ognev

A scheme is proposed for the generation of branch-entangled pairs of microcavity polaritons through spontaneous inter-branch parametric scattering. Branch-entanglement is achievable when there are two twin processes, where the role of…

Mesoscale and Nanoscale Physics · Physics 2009-11-10 Cristiano Ciuti

Photoabsorption by and fluorescence of the K{\alpha} transitions in highly charged iron ions are essential mechanisms for X-ray radiation transfer in astrophysical environments. We study photoabsorption due to the main K{\alpha} transitions…

We show that polarization entangled photons at x-ray energies can be generated via spontaneous parametric down conversion. Each of the four Bell states can be generated by choosing the angle of incidence and polarization of the pumping…

Quantum Physics · Physics 2015-03-17 S. Shwartz , S. E. Harris

We present observational evidence for "propeller" effects in two X-ray pulsars, GX 1+4 and GROJ1744-28. Both sources were monitored regularly by the Rossi X-ray Timing Explorer (RXTE) throughout a decaying period in the X-ray brightness.…

Astrophysics · Physics 2009-10-30 Wei Cui

The highest energy cosmic rays could be produced by drifts in magnetized, cylindrically collimated, sheared jets of powerful active galaxies (i.e. FR II radiogalaxies; radio loud quasars and high power BL Lacs). We show that in such…

Astrophysics · Physics 2007-06-20 Rachid Ouyed , Guenter Sigl , Maxim Lyutikov

While the scientific potential of high-energy X-ray and gamma-ray polarimetry has long been recognized, measuring the polarization of high-energy photons is challenging. To date, there has been very few significant detections from an…

Instrumentation and Methods for Astrophysics · Physics 2023-04-05 Denis Bernard , Tanmoy Chattopadhyay , Fabian Kislat , Nicolas Produit

We propose that neutrons may be generated in high-energy, high-flux photon environments via photo-induced reactions on pre-existing baryons. These photohadronic interactions are expected to occur in astrophysical jets and surrounding…

High Energy Astrophysical Phenomena · Physics 2025-07-08 Matthew R. Mumpower , Tsung-Shung H. Lee , Nicole Lloyd-Ronning , Brandon L. Barker , Axel Gross , Samuel Cupp , Jonah M. Miller

We consider the interaction between radiation, matter and a magnetic field in a compact, relativistic jet. The entrained matter accelerates outward as the jet breaks out of a star or other confining medium. In some circumstances, such as…

High Energy Astrophysical Phenomena · Physics 2015-06-15 Matthew Russo , Christopher Thompson

The presence of radiatively driven outflows is well established in ultraluminous X-ray sources (ULXs). These outflows are optically thick and can reprocess a significant fraction of the accretion luminosity. Assuming isotropic emission,…

High Energy Astrophysical Phenomena · Physics 2021-10-27 Matthew Middleton , Nick Higginbottom , Christian Knigge , Norman Khan , Grzegorz Wiktorowicz

The magnificent development of strong X-ray lasers motivates the advancement of pair production process studies into higher laser frequency region. In this paper, a resonant electron-positron pair production process with the absorption of…

Atomic Physics · Physics 2015-06-17 Huayu Hu , Jie Huang

A fraction of high-mass X-ray binaries are supergiant fast X-ray transients. These systems have on average low X-ray luminosities, but display short flares during which their X-ray luminosity rises by a few orders of magnitude. The leading…

High Energy Astrophysical Phenomena · Physics 2020-02-19 Swetlana Hubrig , Lara Sidoli , Konstantin A. Postnov , Markus Schöller , Alexander F. Kholtygin , Silva P. Jarvinen

Robust generation of gamma-ray bursts (GRBs) implies the formation of outflows with very low baryon loads and highly relativistic velocities, but more baryon-rich, slower outflows are also likely to occur in most GRB central engine…

Astrophysics · Physics 2008-11-26 Susumu Inoue , Nobuyuki Iwamoto , Manabu Orito , Mariko Terasawa

Some of the proposed explanations for the origin of ultrahigh-energy cosmic rays invoke new sources of energetic photons (e.g., topological defects, relic particles, etc.). At high red shift, when the cosmic microwave background has a…

High Energy Physics - Phenomenology · Physics 2009-10-31 Alexander Kusenko , Marieke Postma

Photon pair generation in silicon photonic integrated circuits relies on four wave mixing via the third order nonlinearity. Due to phase matching requirements and group velocity dispersion, this method has typically required TE polarized…