Theoretical astrophysics : an introduction (Record no. 16684)

MARC details
000 -LEADER
fixed length control field 02179nam a2200289Ia 4500
003 - CONTROL NUMBER IDENTIFIER
control field OSt
005 - DATE AND TIME OF LATEST TRANSACTION
control field 20260123112226.0
008 - FIXED-LENGTH DATA ELEMENTS--GENERAL INFORMATION
fixed length control field 220909b |||||||| |||| 00| 0 eng d
020 ## - INTERNATIONAL STANDARD BOOK NUMBER
International Standard Book Number 9783527410040
037 ## - SOURCE OF ACQUISITION
Terms of availability Textbook
040 ## - CATALOGING SOURCE
Original cataloging agency CSL
Language of cataloging eng
Transcribing agency CSL
041 ## - LANGUAGE CODE
Language code of text/sound track or separate title eng
084 ## - COLON CLASSIFICATION NUMBER
Classification number B9:6 Q3 TC
Assigning agency CSL
100 ## - MAIN ENTRY--PERSONAL NAME
Personal name Bartelmann, Matthias
9 (RLIN) 1104715
245 #0 - TITLE STATEMENT
Title Theoretical astrophysics : an introduction
260 ## - PUBLICATION, DISTRIBUTION, ETC.
Place of publication, distribution, etc. Weinheim,
Name of publisher, distributor, etc. Wiley-VCH:
Date of publication, distribution, etc. 2013.
300 ## - PHYSICAL DESCRIPTION
Extent xx,320p.
Other physical details : col. ill.
490 ## - SERIES STATEMENT
Series statement Physics textbook
500 ## - GENERAL NOTE
General note Include bibliographical references.; Index 315-320p.
520 ## - SUMMARY, ETC.
Summary, etc. Beginning from first principles and adopting a modular structure, this book develops the fundamental physical methods needed to describe and understand a wide range of seemingly very diverse astrophysical phenomena and processes. For example, the discussion of radiation processes including their spectra is based on Larmor's equation and extended by the photon picture and the internal dynamics of radiating quantum systems, leading to the shapes of spectral lines and the ideas of radiation transport. Hydrodynamics begins with the concept of phase-space distribution functions and Boltzmann's equation and develops ideal, viscous and magneto-hydrodynamics all from the vanishing divergence of an energy-momentum tensor, opening a natural extension towards relativistic hydrodynamics. Linear stability analysis is introduced and used as a common and versatile tool throughout the book.<br/>Aimed at students at graduate level, lecturers teaching courses in theoretical astrophysics or advanced topics in modern astronomy, this book with its abundant examples and exercises also serves as a reference and an entry point for more advanced researchers wanting to update their knowledge of the physical processes that govern the behavior and evolution of astronomical objects.
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical term or geographic name entry element Astrophysics
9 (RLIN) 1104716
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical term or geographic name entry element Hydrodynamics
9 (RLIN) 1104717
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical term or geographic name entry element Stellar dynamics
9 (RLIN) 1104718
650 ## - SUBJECT ADDED ENTRY--TOPICAL TERM
Topical term or geographic name entry element Physics
9 (RLIN) 1104719
942 ## - ADDED ENTRY ELEMENTS (KOHA)
Classification part B9:6 Q3 TC
Koha item type Textbook
Source of classification or shelving scheme Colon Classification (CC)
Suppress in OPAC No
Holdings
Withdrawn status Lost status Source of classification or shelving scheme Damaged status Not for loan Home library Current library Date acquired Source of acquisition Total Checkouts Full call number Barcode Date last seen Price effective from Koha item type
    Colon Classification (CC)     Central Science Library Central Science Library 2022-09-12 2281, 07/02/2014, Ashutosh Technical Books   B9:6 Q3 TC SL1560687 2022-09-12 2022-09-12 Textbook
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