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Problems in the Analysis of Gamma-ray Burst Spectra

Problems in the Analysis of Gamma-ray Burst Spectra PDF Author:
Publisher:
ISBN:
Category :
Languages : en
Pages :

Book Description
Spectral measurements by the Solar Maximum Mission have been used to confirm the cyclotron lines in gamma-ray bursts reported from the Konus experiment. We present ISEE-3 data for the same burst (GB800419) during the same period of time which show no line. We discuss various problems in the analysis of scintillator spectra and point out that unfolded spectra are not necessarily unique and that the position of a data point in a deconvolved spectrum may vary depending on the assumed overall shape of the spectrum. As a result, if the analysis assumes a soft spectrum (such as optically thin thermal bremsstrahlung) an absorption feature might appear, whereas a harder spectrum (such as a Comptonized blackbody) would not require the feature. Since the continuum shape probably changes during the duration of a typical burst, the nonuniqueness of the spectral unfolding, combined with the assumption that the continuum is optically thin thermal bremsstrahlung, could give rise to spurious absorption features which vary on a time scale of seconds. Despite these problems, there is still some evidence for narrow spectral lines in the range 45 to 65 keV but not for the broad lines reported from the Konus experiment. Unfortunately, the range 45 to 65 keV is the most difficult spectral region to unfold.

Problems in the Analysis of Gamma-ray Burst Spectra

Problems in the Analysis of Gamma-ray Burst Spectra PDF Author:
Publisher:
ISBN:
Category :
Languages : en
Pages :

Book Description
Spectral measurements by the Solar Maximum Mission have been used to confirm the cyclotron lines in gamma-ray bursts reported from the Konus experiment. We present ISEE-3 data for the same burst (GB800419) during the same period of time which show no line. We discuss various problems in the analysis of scintillator spectra and point out that unfolded spectra are not necessarily unique and that the position of a data point in a deconvolved spectrum may vary depending on the assumed overall shape of the spectrum. As a result, if the analysis assumes a soft spectrum (such as optically thin thermal bremsstrahlung) an absorption feature might appear, whereas a harder spectrum (such as a Comptonized blackbody) would not require the feature. Since the continuum shape probably changes during the duration of a typical burst, the nonuniqueness of the spectral unfolding, combined with the assumption that the continuum is optically thin thermal bremsstrahlung, could give rise to spurious absorption features which vary on a time scale of seconds. Despite these problems, there is still some evidence for narrow spectral lines in the range 45 to 65 keV but not for the broad lines reported from the Konus experiment. Unfortunately, the range 45 to 65 keV is the most difficult spectral region to unfold.

Analysis of Gamma-ray Burst Energy Spectra

Analysis of Gamma-ray Burst Energy Spectra PDF Author:
Publisher:
ISBN:
Category :
Languages : en
Pages : 3

Book Description
This report summarizes the work carried out under LLNL Contract Number B108527, subcontracted by the Regents of the University of California at Berkeley. The research carried out under this contract includes assisting in the data analysis for the Prognoz-9 mission, linking results of the computer codes to the Prognoz-9 data library in order to study the spectral shape and evolution of cosmic gamma-ray burst energy spectra, and using the results of this study to help to determine or constrain the physical conditions at the gamma-ray bursts sources. The results of this work led to several publications that have shed considerable insight into the gamma-ray burst mystery, and gives a new diagnostic for determining the nature of gamma-ray burst sources. The outcome of this work also provides a new spectral form for studying the temporal evolution and spectral behavior of gamma-ray bursts.

A Study of the Temporal and Spectral Characteristics of Gamma Ray Bursts

A Study of the Temporal and Spectral Characteristics of Gamma Ray Bursts PDF Author: Jay Preston Norris
Publisher:
ISBN:
Category : Gamma ray astronomy
Languages : en
Pages : 570

Book Description


The Physics of Gamma-Ray Bursts

The Physics of Gamma-Ray Bursts PDF Author: Bing Zhang
Publisher: Cambridge University Press
ISBN: 1107027616
Category : History
Languages : en
Pages : 617

Book Description
A complete text on the physics of gamma-ray bursts, the most brilliant explosions since the Big Bang.

Practical Gamma-ray Spectroscopy

Practical Gamma-ray Spectroscopy PDF Author: Gordon Gilmore
Publisher: John Wiley & Sons
ISBN: 1119964695
Category : Science
Languages : en
Pages : 597

Book Description
The Second Edition of Practical Gamma-Ray Spectrometry has been completely revised and updated, providing comprehensive coverage of the whole gamma-ray detection and spectrum analysis processes. Drawn on many years of teaching experience to produce this uniquely practical volume, issues discussed include the origin of gamma-rays and the issue of quality assurance in gamma-ray spectrometry. This new edition also covers the analysis of decommissioned nuclear plants, computer modelling systems for calibration, uncertainty measurements in QA, and many more topics.

Gamma-Ray Bursts

Gamma-Ray Bursts PDF Author: Gilbert Vedrenne
Publisher: Springer Science & Business Media
ISBN: 354039088X
Category : Science
Languages : en
Pages : 613

Book Description
Since their discovery was first announced in 1973, gamma-ray bursts (GRBs) have been among the most fascination objects in the universe. While the initial mystery has gone, the fascination continues, sustained by the close connection linking GRBs with some of the most fundamental topics in modern astrophysics and cosmology. Both authors have been active in GRB observations for over two decades and have produced an outstanding account on both the history and the perspectives of GRB research.

Gamma-ray Bursts

Gamma-ray Bursts PDF Author: Cheng Ho
Publisher: Cambridge University Press
ISBN: 9780521414494
Category : Nature
Languages : en
Pages : 532

Book Description
Summarizes the current understanding of Astronomical gamma-ray bursts, short-lived flashes of high-energy radiation, which have eluded even a basic explanation for over twenty years, and describes directions for future research.

Magnetic Fields in Diffuse Media

Magnetic Fields in Diffuse Media PDF Author: Alexander Lazarian
Publisher: Springer
ISBN: 3662446251
Category : Science
Languages : en
Pages : 627

Book Description
This volume presents the current knowledge of magnetic fields in diffuse astrophysical media. Starting with an overview of 21st century instrumentation to observe astrophysical magnetic fields, the chapters cover observational techniques, origin of magnetic fields, magnetic turbulence, basic processes in magnetized fluids, the role of magnetic fields for cosmic rays, in the interstellar medium and for star formation. Written by a group of leading experts the book represents an excellent overview of the field. Nonspecialists will find sufficient background to enter the field and be able to appreciate the state of the art.

A Temporal and Spectral Analysis of Gamma-ray Bursts Observed with BATSE

A Temporal and Spectral Analysis of Gamma-ray Bursts Observed with BATSE PDF Author: Timothy W. Giblin
Publisher:
ISBN:
Category : Gamma ray bursts
Languages : en
Pages : 438

Book Description


Pattern Recognition with Fuzzy Objective Function Algorithms

Pattern Recognition with Fuzzy Objective Function Algorithms PDF Author: James C. Bezdek
Publisher: Springer Science & Business Media
ISBN: 147570450X
Category : Mathematics
Languages : en
Pages : 267

Book Description
The fuzzy set was conceived as a result of an attempt to come to grips with the problem of pattern recognition in the context of imprecisely defined categories. In such cases, the belonging of an object to a class is a matter of degree, as is the question of whether or not a group of objects form a cluster. A pioneering application of the theory of fuzzy sets to cluster analysis was made in 1969 by Ruspini. It was not until 1973, however, when the appearance of the work by Dunn and Bezdek on the Fuzzy ISODATA (or fuzzy c-means) algorithms became a landmark in the theory of cluster analysis, that the relevance of the theory of fuzzy sets to cluster analysis and pattern recognition became clearly established. Since then, the theory of fuzzy clustering has developed rapidly and fruitfully, with the author of the present monograph contributing a major share of what we know today. In their seminal work, Bezdek and Dunn have introduced the basic idea of determining the fuzzy clusters by minimizing an appropriately defined functional, and have derived iterative algorithms for computing the membership functions for the clusters in question. The important issue of convergence of such algorithms has become much better understood as a result of recent work which is described in the monograph.