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Related papers: Steep Decay Phase Shaped by the Curvature Effect. …

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We derive a simple analytical formula to describe the evolution of spectral index $\beta$ in the steep decay phase shaped by the curvature effect with assumption that the spectral parameters and Lorentz factor of jet shell is the same for…

High Energy Astrophysical Phenomena · Physics 2017-05-24 Da-Bin Lin , Hui-Jun Mu , Yun-Feng Liang , Tong Liu , Wei-Min Gu , Rui-Jing Lu , Xiang-Gao Wang , En-Wei Liang

The curvature effect is explored in the case of extremely short intrinsic emission. Assuming a $\delta$ function emission we get formulas that get rid of the impacts from the intrinsic emission duration, which are applicable to any forms of…

Astrophysics · Physics 2011-02-11 Y. -P. Qin

As a result of spherical kinematics, temporal evolution of received gamma-ray emission should demonstrate signatures of curvature from the emitting shell. Specifically, the shape of the pulse decay must bear a strict dependence on the…

Astrophysics · Physics 2009-11-06 Alicia M. Soderberg , Edward E. Fenimore

Spectral evolution of gamma-ray burst pulses assumed to arise from emission of fireballs is explored. It is found that, due to the curvature effect, the integrated flux and peak energy are well related by a power law in the decaying phase…

High Energy Astrophysical Phenomena · Physics 2009-11-13 Y. -P. Qin

We study the impact of a temperature-dependent curvaton decay rate on the primordial curvature perturbation generated in the curvaton scenario. Using the familiar sudden decay approximation, we obtain an analytical expression for the…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-22 Naoya Kitajima , David Langlois , Tomo Takahashi , Tomohiro Takesako , Shuichiro Yokoyama

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

We present a numerical method for computing the evolution of a planar, star-shaped curve under a broad class of curvature-driven geometric flows, which we refer to as the Andrews-Bloore flows. This family of flows has two parameters that…

Dynamical Systems · Mathematics 2020-10-22 Eszter Fehér , Gábor Domokos , Bernd Krasukopf

When emission in a conical relativistic jet ceases abruptly (or decays sharply), the observed decay light curve is controlled by the high-latitude "curvature effect". Recently, Uhm & Zhang found that the decay slopes of three GRB X-ray…

High Energy Astrophysical Phenomena · Physics 2016-08-03 Lan-Wei Jia , Z. Lucas Uhm , Bing Zhang

(abridged) Aims: To study turbulent transport coefficients that describe the evolution of large-scale magnetic fields in turbulent convection. Methods: We use the test field method together with 3D numerical simulations of turbulent…

Astrophysics · Physics 2009-07-29 P. J. Käpylä , M. J. Korpi , A. Brandenburg

We obtain a remarkable semi-analytic expression concerning the role of purely tidal curvature on accelerated probes, revealing some novel insights into the role of absolute vs. tidal acceleration in the response of such probes. The key…

General Relativity and Quantum Cosmology · Physics 2021-10-22 Hari K , Dawood Kothawala

Time evolution of the decay process of unstable particles is investigated in field theory models. We first formulate how to renormalize the non-decay amplitude beyond perturbation theory and then discuss short-time behavior of very…

High Energy Physics - Phenomenology · Physics 2009-10-30 I. Joichi , Sh. Matsumoto , M. Yoshimura

We consider a relativistic spherical shell and calculate its spectral flux as received by a distant observer. Using two different methods, we derive a simple analytical expression of the observed spectral flux and show that the well-known…

High Energy Astrophysical Phenomena · Physics 2015-08-06 Z. Lucas Uhm , Bing Zhang

The dynamics of a passive scalar plume in a turbulent boundary layer is experimentally investigated via vertical turbulent transport time-series. Data are acquired in a rough-wall turbulent boundary layer that develops in a recirculating…

We introduce a new method for detecting scaling in time series. The method uses the properties of the probability flux for stochastic self-affine processes and is called the probability flux analysis (PFA). The advantages of this method…

Data Analysis, Statistics and Probability · Physics 2010-04-05 M. Ignaccolo , P. Grigolini , B. J. West

The time-dependent analysis of the decays $\Lambda_b\to \Lambda +D^0(t)$ and $\Lambda_b\to \Lambda +\bar{D}^0(t)$ is discussed. The effect of particle mixing due to time evolution of $D^0$ and $\bar{D}^0$ on the observables for these decays…

High Energy Physics - Phenomenology · Physics 2007-05-23 Fayyazuddin

As revealed previously, under the assumption that some pulses of gamma-ray bursts are produced by shocks in spherical fireballs or uniform jets of large opening angles, there exists a standard decay form of the profile of pulses arising…

Astrophysics · Physics 2008-11-26 Y. -P. Qin , R. -J. Lu

We use the local curvature derived from velocity vector fields or particle tracks as a surrogate for structure size to compute curvature-based energy spectra. An application to homogeneous isotropic turbulence shows that these spectra…

The scaling ranges of time correlations in the cloud base height records of marine boundary layer stratocumulus are studied applying the Detrended Fluctuation Analysis statistical method. We have found that time dependent variations in the…

Condensed Matter · Physics 2009-11-07 N. Kitova , K. Ivanova , M. Ausloos , T. P. Ackerman , M. A. Mikhalev

If more than one curvaton dominate the Universe at different epochs from each other, curvature perturbations can be temporarily enhanced to a value much larger than the observed one 10^{-5}. The traces of the enhancement may be left as…

Cosmology and Nongalactic Astrophysics · Physics 2013-05-29 Teruaki Suyama , Jun'ichi Yokoyama

We analyze the time profiles of individual gamma-ray burst (GRB) pulses, that are longer than 2 s, by modelling them with analytical functions that are based empirical descriptions of GRB spectral evolution. These analytical profiles are…

Astrophysics · Physics 2009-11-07 Dan Kocevski , Felix Ryde , Edison Liang
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