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Related papers: Time duration of the parametric x-ray radiation

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We investigate the two-particle interferometry for the particle-emitting sources which undergo the first-order phase transition from the quark-gluon plasma with a finite baryon chemical potential to hadron resonance gas. The effects of…

Nuclear Theory · Physics 2013-05-30 Hong-Jie Yin , Jing Yang , Wei-Ning Zhang , Li-Li Yu

To shorten the duration of x-ray pulses, we present a nonlinear optical technique using atoms with core-hole vacancies (core-hole atoms) generated by inner-shell photoionization. The weak Coulomb screening in the core-hole atoms results in…

We studied the evolution of the X-ray and gamma-ray spectra of the Crab pulsar utilizing the 11-year observations from the Rossi X-ray Timing Explorer (RXTE) and 9-year observations from the Fermi Gamma-ray Space Telescope (FGST). By…

High Energy Astrophysical Phenomena · Physics 2018-10-10 L. L. Yan , M. Y. Ge , F. J. Lu , S. J. Zheng , Y. L. Tuo , Z. J. Li , L. M. Song , J. L. Qu

Laser-plasma acceleration is an emerging technique for accelerating electrons to high energies over very short distances. The accelerated electron bunches have femtosecond duration, making them particularly relevant for applications such as…

The understanding of pulsar radio emission demands a close look at all regions of the huge parameter space present for pulsar observations. In this review we concentrate on the space given by the range of observed pulse periods, spanning…

Astrophysics · Physics 2007-05-23 M. Kramer

The radio millisecond pulsar PSR J1023+0038 exhibits complex timing and eclipse behavior. Here we analyze four years' worth of radio monitoring observations of this object. We obtain a long-term timing solution, albeit with large residual…

High Energy Astrophysical Phenomena · Physics 2013-11-21 Anne M. Archibald , Victoria M. Kaspi , Jason W. T. Hessels , Ben Stappers , Gemma Janssen , Andrew Lyne

We show that when a supernova explodes, a nearby pulsar signal goes through a very specific change. The observed period first changes smoothly, then is followed by a sudden change in the time derivative. A stable millisecond pulsar can…

High Energy Astrophysical Phenomena · Physics 2016-06-01 Darsh Kodwani , Ue-Li Pen , I-Sheng Yang

Determining the pulse duration of femtosecond electron bunches is challenging and often experimentally invasive. An effective method for measuring the duration based on the time-dependent variations in electron beam divergence induced by a…

Accelerator Physics · Physics 2025-07-01 Andreas Seidel , Carola Zepter , Alexander Sävert , Stephan Kuschel , Matt Zepf

For the first time, the consequences of combining two well-established empirical relations, describing different aspects of the spectral evolution of observed gamma-ray burst (GRB) pulses, are explored. These empirical relations are: i) the…

Astrophysics · Physics 2009-10-31 Felix Ryde , Roland Svensson

Superluminal tunneling of light through a barrier has attracted broad interest in the last several decades. Despite the observation of such phenomena in various systems, it has been under intensive debate whether the transmitted light truly…

Optics · Physics 2021-04-06 Liang Wu , Zhiyong Wang , Kai Kang1 , Yi Fu , Chuanwei Li1 , Weili Zhang , Shuang Zhang

The origin of a part of the single pulsars with relatively low magnetic fields B < 1E12 G and with characteristic times Tau < 1E7 yr is established. Such pulsars occur as a result of the disruption of High Mass X-ray Binary Systems after a…

Astrophysics · Physics 2009-11-10 O. H. Guseinov , A. O. Allakhverdiev , S. Tagieva , O. Taskin

We investigate structure and evolution of long positive spark breakdown; and we study at which stage pulses of hard X-rays are emitted. Positive high-voltage pulses of standardized lightning impulse wave form of about 1 MV were applied to…

Plasma Physics · Physics 2015-03-13 P. O. Kochkin , C. V. Nguyen , A. P. J. van Deursen , U. Ebert

Theoretical aspects of x-ray standing wave method for investigation of the real structure of crystals are considered in this review paper. Starting from the general approach of the secondary radiation yield from deformed crystals this…

Materials Science · Physics 2015-06-24 I. A. Vartanyants , M. V. Kovalchuk

We report the discovery of a systematic constant time lag between the X-ray and radio flares of the gamma-ray binary LSI +61 303, persistent over long, multi-year, time scale. Using the data of monitoring of the system by RXTE we show that…

High Energy Astrophysical Phenomena · Physics 2012-03-12 M. Chernyakova , A. Neronov , S. Molkov , D. Malyshev , A. Lutovinov , G. Pooley

We use numerical modeling to study the features of parametric (quasi-Cherenkov) cooperative radiation arising when an electron bunch passes through a crystal (natural or artificial) under the conditions of dynamical diffraction of…

Accelerator Physics · Physics 2013-04-04 S. V. Anishchenko , V. G. Baryshevsky

We observed periodic optical pulses from an Er:YSO crystal during irradiating with an continuous-wave excitation laser. We refer to this new phenomenon as "periodic super-radiance". This periodicity can be understood qualitatively by a…

In strict analogy to prompt pulses, X-ray flares observed by Swift-XRT in long Gamma-Ray Bursts define a lag-luminosity relation: L_p,iso \propto t_lag^{-0.95+/-0.23}. The lag-luminosity is proven to be a fundamental law extending 5 decades…

High Energy Astrophysical Phenomena · Physics 2015-05-19 R. Margutti

The multiple scattering effect on the line width of the backward Parametric X-ray Radiation (PXR) in the extremely Bragg geometry, produced by low energy relativistic electrons traversing a single crystal, is discussed. It is shown that…

Accelerator Physics · Physics 2015-02-09 Mehdi Tabrizi

Based on kinematic model of parametric X-ray Radiation (PXR), an approach for calculation of PXR characteristics (spectrum, intensity, polarization and yield) has been developed. The approach allows to take into account the beam divergence,…

Strongly Correlated Electrons · Physics 2016-08-31 A. P. Potylitsin
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