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A lot of beautiful observations of Supernova remnant 1987A give a precise idea of its structure and its evolution. The regular interpretations of the observations set that the large energy needed to explain the brightness of the pearl…

综合物理 · 物理学 2007-05-23 Jacques Moret-Bailly

We discuss the X-ray emission observed from Supernova Remnant 1987A with the Chandra X-ray Observatory. We analyze a high resolution spectrum obtained in 1999 October with the high energy transmission grating (HETG). From this spectrum we…

We study the peripheral ion collisions at LHC energies in which a nucleus is excited to the discrete state and then emits $\gamma$-rays. Large nuclear Lorenz factor allows to observe the high energy photons up to a few ten GeV and in the…

核理论 · 物理学 2009-11-10 Yu. V. Kharlov , V. L. Korotkikh

Turbulent radiation flow is commonplace in systems with strong, incoherent, light-matter interactions. In astrophysical contexts, photon bubble turbulence is considered a key mechanism behind enhanced radiation transport, and its importance…

原子物理 · 物理学 2021-07-06 R. Giampaoli , João D. Rodrigues , José A. Rodrigues , José T. Mendonça

We report on the discovery of a shell-type supernova remnant in the southern sky. It is a large (8*8), low-brightness source with a nonthermal radio spectrum, which requires background filtering to isolate it from the diffuse background…

天体物理学 · 物理学 2009-11-06 Jorge A. Combi , Gustavo E. Romero , Paula Benaglia , Justin L. Jonas

Radiation by the atoms of a resonant medium is a cooperative process in which the medium participates as a whole. In two previous papers \cite{PG00,GP00}, we treated this problem for the case of a medium having slab geometry, which, under…

光学 · 物理学 2015-05-20 Sudhakar Prasad , Roy J. Glauber

Dark photon dark matter will resonantly convert into visible photons when the dark photon mass is equal to the plasma frequency of the ambient medium. In cosmological contexts, this transition leads to an extremely efficient, albeit…

宇宙学与河外天体物理 · 物理学 2020-07-15 Samuel J. Witte , Salvador Rosauro-Alcaraz , Samuel D. McDermott , Vivian Poulin

We point out a few remarkable properties of the $\gamma\gamma\to\gamma\gamma$ process at high energy. They should allow to search for effects of new particles and interactions. We give illustrations with threshold effects due to pairs of…

高能物理 - 唯象学 · 物理学 2009-10-31 G. J. Gounaris , P. I. Porfyriadis , F. M. Renard

There has recently been interest in the role of inverse bremsstrahlung, the emission of photons by fast suprathermal ions in collisions with ambient electrons possessing relatively low velocities, in tenuous plasmas in various astrophysical…

天体物理学 · 物理学 2009-10-31 Matthew G. Baring , Frank C. Jones , Donald C. Ellison

The low energy spectral slopes of the prompt emission of most gamma-ray bursts (GRBs) are difficult to reconcile with radiatively efficient optically thin emission models irrespective of the radiation mechanism. An alternative is to ascribe…

高能天体物理现象 · 物理学 2015-06-11 Indrek Vurm , Yuri Lyubarsky , Tsvi Piran

We analyze the obtained solutions of the non-linear Shroedinger equation for spherically and axially symmetrical electrons density oscillations in plasma. The conditions of the oscillations process existence are examined. It is shown that…

等离子体物理 · 物理学 2009-07-31 Maxim Dvornikov , Sergey Dvornikov

Coherent light sources, such as free electron lasers, provide bright beams for biology, chemistry, physics, and advanced technological applications. Increasing the brightness of these sources requires progressively larger devices, with the…

等离子体物理 · 物理学 2023-01-27 B. Malaca , M. Pardal , D. Ramsey , J. Pierce , K. Weichman , I. Andriyash , W. B. Mori , J. P. Palastro , R. A. Fonseca , J. Vieira

Ionization by relativistically intense short laser pulses is studied in the framework of strong-field quantum electrodynamics. Distinctive patterns are found in the energy probability distributions of photoelectrons. Except of the already…

原子物理 · 物理学 2018-03-14 F. Cajiao Vélez , J. Z. Kamiński , K. Krajewska

Bubble formation in liquid xenon underneath a Thick Gaseous Electron Multiplier (THGEM) electrode immersed in liquid xenon was observed with a CCD camera. With voltage across the THGEM, the appearance of bubbles was correlated with that of…

仪器与探测器 · 物理学 2015-09-09 E. Erdal , L. Arazi , V. Chepel , M. L. Rappaport , D. Vartsky , A. Breskin

Photon spheres, surfaces where massless particles are confined in closed orbits, are expected to be common astrophysical structures surrounding ultracompact objects. In this paper a semiclassical treatment of a photon sphere is proposed. We…

广义相对论与量子宇宙学 · 物理学 2014-11-24 M. C. Baldiotti , Walace S. Elias , C. Molina , Thiago S. Pereira

Numerous sources produce the ionization impact on the planetary atmosphere. The tropospheric cloudiness therewith is originated at such altitudes, which coincide with places of the maximum of the atmospheric ionization that caused by space…

等离子体物理 · 物理学 2024-02-06 N. I. Izhovkina , S. N. Artekha , N. S. Erokhin , L. A. Mikhailovskaya

Electrons at the surface of a plasma that is irradiated by a laser with intensity in excess of $10^{23}~\mathrm{W}\mathrm{cm}^{-2}$ are accelerated so strongly that they emit bursts of synchrotron radiation. Although the combination of high…

等离子体物理 · 物理学 2021-05-12 T. G. Blackburn , A. J. MacLeod , A. Ilderton , B. King , S. Tang , M. Marklund

Sonoluminescence is the intriguing phenomenon of strong light flashes from tiny bubbles in a liquid. The bubbles are driven by an ultrasonic wave and need to be filled with noble gas atoms. Approximating the emitted light by blackbody…

其他凝聚态物理 · 物理学 2009-06-19 Andreas Kurcz , Antonio Capolupo , Almut Beige

We study the interaction of intense ultrashort laser pulses with cryogenic He jets using 2d/3v relativistic Particle-in-Cell simulations (XOOPIC). Of particular interest are laser intensities $(10^{15}-10^{20})$ W/cm$^2$, pulse lengths $\le…

等离子体物理 · 物理学 2017-04-05 M. Shihab , T. Bornath , R. Redmer

We investigate the importance of the pseudo-continuum bound-free opacity from hydrogen atoms in the atmospheres of cool white dwarfs. This source of absorption, when calculated by the occupation probability formalism applied in the modeling…

天体物理学 · 物理学 2008-11-26 Piotr M. Kowalski