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4 edition of Nuclear spectroscopy of astrophysical sources found in the catalog.

Nuclear spectroscopy of astrophysical sources

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Published by American Institute of Physics in New York .
Written in English


Edition Notes

Statementedited by Neil Gehrels and Gerald H. Share.
SeriesAIP conference proceedings -- no. 170
ID Numbers
Open LibraryOL20819366M
ISBN 100883183706

  Astrophysics is a branch of space science that applies the laws of physics and chemistry to explain the birth, life and death of stars, planets, galaxies, nebulae and other objects in the : Ariel Balter. COMPACT STELLAR X-RAY SOURCES X-ray astronomy provides the main window onto astrophysical compact objects such as black holes, neutron stars and white dwarfs. In the past ten years new observational opportunities have led to an explosion of knowledge in this field. In sixteen chapters,File Size: KB.

‘The book is really a treasure for any student and teacher interested in astrophysics. It is very up to date and synoptically covers the whole field of high-energy astrophysics. I will use the book for my lectures as soon as I can!’ Günther Hasinger - Scientific Director, Max-Planck-Institut für PlasmaphysikCited by: @article{osti_, title = {Flux and spectrum of reactor antineutrinos}, author = {Kopeikin, V. I., E-mail: [email protected]}, abstractNote = {In order to perform reactor experiments aimed at studying the nature of the neutrino and measurements in the realms of geo- and astrophysical neutrinos and to meet practical requirements in this field, it is highly desirable to obtain deeper.

Member Scientific Organizing Committee, Workshop on Nuclear Spectroscopy of Astrophysical Sources", Washington DC, December, , Presented invited paper on "The Production of Candidates for Gamma-Line Astronomy in Astrophysical Explosions", to be published in the Proceedings. This book, presented in two volumes, discusses the papers on nuclear structure and symmetries. The topics of discussion were octupole and dipole modes, interacting boson version of reflection-asymmetric deformation, alpha decay of actinide nuclei, experimental studies of symmetries, high spin physics, theory of unified nuclei, odd-even nuclei, boson densities by electron scattering, symmetries.


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Nuclear spectroscopy of astrophysical sources Download PDF EPUB FB2

Book-Review - Nuclear Spectroscopy of Astrophysical Sources The ADS is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative Agreement NNX16AC86A. Resources About ADS ADS Help What's New [email protected] Social @adsabs.

Get this from a library. Nuclear spectroscopy of astrophysical sources: Washington, D.C., [Neil Gehrels; Gerald H Share;].

The IOP Series in Nuclear Spectroscopy and Nuclear Structure provides up-to-date coverage of theoretical and experimental topics in all areas of modern nuclear spectroscopy and structure. Books in the series range from student primers, graduate textbooks, research monographs and practical guides to meet the needs of students and scientists.

Reset your password. If you have a user account, you will need to reset your password the next time you login. You will only need to do this once. Book Review: Nuclear spectroscopy. RACAH (editor) (International School of Physics "E. Fermi", Varenna) (Academic Press. New York, viii p.

$ ). nuclear power and propulsion for specific astrophysical applications To gauge the possibility that radioisotope power systems (RPSs) and/or fission reactors might enhance or enable the achievement of important astrophysical goals, this chapter examines several types of astrophysical missions for which nuclear systems might potentially be.

Natural sources of gamma rays on Earth include gamma decay from naturally occurring radioisotopes such as potassium, and also as a secondary radiation from various atmospheric interactions with cosmic ray particles. Some rare terrestrial natural sources that produce gamma rays that are not of a nuclear origin, are lightning strikes and terrestrial gamma-ray flashes, which produce high.

Abstract. The discovery (Matz et al. [1]) of gamma-ray line emission at and keV from radioactive 56 Co in the recent supernova SNA proved that explosive nucleosynthesis occurred in this supernova.

Gamma-ray light curves derived from these and subsequent observations (Cook et al. [2], Mahoney et al. [3], Sandie et al. [4], Rester et al. [5], Teegarden et al. [6]) have a broad Author: J. Matteson, M. Felling, B. Bowman, M. Briggs, R. Lingenfelter, L. Peterson, R. Lin, D. Smith, K. Astrophysical gamma-ray spectroscopy is an invaluable tool for studying nuclear astrophysics, supernova structure, recent star formation in the Milky Way and mixing of nucleosynthesis products in.

This book covers the following topics: Definitions of and Relations between Quantities used in Radiation Theory, Blackbody Radiation, The Exponential Integral Function, Flux, Specific Intensity and other Astrophysical Terms, Absorption, Scattering, Extinction and the Equation of Transfer, Limb Darkening, Atomic Spectroscopy, Boltzmann's and.

The book serves both as a textbook, with many examples and end-of-chapter exercises, but also as a reference book for use by researchers working in the field of nuclear astrophysics. View Show. Fundamentals in nuclear physics: from nuclear structure to cosmology Jean-Louis Basdevant, James Rich, Michael Spiro This course on nuclear physics leads the reader to the exploration of the field from nuclei to astrophysical issues.

NuSTAR (Nuclear Spectroscopic Telescope Array) is a space-based X-ray telescope that uses a conical approximation to a Wolter telescope to focus high energy X-rays from astrophysical sources, especially for nuclear spectroscopy, and operates in the range of 3 to 79 keV.

NuSTAR is the eleventh mission of NASA's Small Explorer satellite program (SMEX) and the first space-based direct-imaging Mission type: X-ray astronomy. This book gives a comprehensive treatment of plasma spectroscopy, the quantitative study of line and continuous radiation from high temperature plasmas.

This highly interdisciplinary field combines elements of atomic, plasma and statistical physics, and has wide application to simulations and diagnostics of laboratory and astrophysical plasmas.

Mahoney: in Nuclear Spectroscopy of Astrophysical Sources, eds. Gehrels and G.H. Share (AIP, New York, ) p. Google ScholarCited by: 4. A convenient single volume handbook featuring the most important topics in spectroscopy This valuable handbook is based on topics presented in the CRC Handbook of Spectroscopy, Volumes I and II, published inand Volume III, published in Tilo Seydel, in Experimental Methods in the Physical Sciences, Proteins as Hydrated Powders.

The roles of the proteins and their hydration water are closely interconnected and have been subject to experimental studies using neutron, nuclear magnetic resonance, and Terahertz spectroscopy [].In particular, the molecular dynamics of hydrated protein powder samples as a function of.

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; Galaxy Formation. This book is a reference in the field of astrophysics with radioactive isotopes including latest results in nuclear astrophysics. It also discusses new windows of astronomy that have been opened up in recent years: neutrinos astronomy, gravitational waves astronomy, asteroseismology.

This is a rather fundamental result that shows the importance of spectroscopy for the interpretation of astrophysical observations. In fact, only the determination of the transition frequency for p -H 2 D + at THz measured in the laboratory several years before by means of new techniques of ion spectroscopy enabled this discovery [ 59 ].Cited by: 2.

NUCLEAR REACTIONS FOR ASTROPHYSICS Principles, Calculation andApplications of Low-Energy Reactions Nuclear processes in stars produce the chemical elements for planets and book shows how similar processes may be reproduced in laboratories using exotic beams, and how these results can be analyzed.The Fundamentals of Stellar Astrophysics.

This book covers the following topics: Introduction and Fundamental Principles, Basic Assumptions, Theorems, and Polytropes, Sources and Sinks of Energy, Flow of Energy through the Star and Construction of Stellar Models, Theory of Stellar Evolution, Relativistic Stellar Structure, Structure of Distorted Stars, Stellar Pulsation and Oscillation, The.Atomic and Molecular Spectroscopy is a wide-ranging review of modern spectroscopic techniques such as X-ray, photoelectron, optical and laser spectroscopy, and radiofrequency and microwave techniques.

On the fundamental side it focuses on physical principles and the impact of spectroscopy on our understanding of the building blocks of matter, while in the area of applications particular 5/5(1).