Astrophysical Formulae: Volume I & Volume II: Radiation, Gas Processes and High Energy Astrophysics / Space, Time, Matter and Cosmology

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Springer Science & Business Media, 22 de febr. 2006 - 1054 pàgines

Kenneth Lang's classic work Astrophysical Formulae. (Vol. I and II) is now available as soft cover edition in a set.

This volume is a reference source of fundamental formulae in physics and astrophysics. In contrast to most of the usual compendia it carefully explains the physical assumptions entering the formulae. All the important results of physical theories are covered: electrodynamics, hydrodynamics, general relativity, atomic and nuclear physics, and so on. Over 2100 formulae are included, and the original papers for the formulae are cited together with papers on modern applications in a bibliography of over 1900 entries. For the third edition (first published in 1999), a chapter on space, time, matter and cosmology had been included and the other chapters carefully revised.

 

Continguts

I
4
IV
5
V
11
VI
13
VII
22
IX
24
X
26
XI
27
XXXI
121
XXXII
123
XXXIII
134
XXXIV
143
XXXV
147
XXXVI
167
XXXVII
176
XXXVIII
183

XII
35
XIII
40
XIV
45
XV
67
XVII
68
XVIII
71
XIX
72
XX
76
XXI
78
XXII
80
XXIII
83
XXIV
100
XXV
105
XXVI
107
XXVII
112
XXIX
114
XXX
116
XL
195
XLI
212
XLII
226
XLIV
232
XLV
238
XLVI
247
XLVII
267
XLVIII
275
L
287
LI
295
LII
300
LIII
308
LIV
317
LV
393
LVI
407
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Passatges populars

Pàgina 3 - A luminous star, of the same density as the Earth, and whose diameter should be two hundred and fifty times larger than that of the Sun, would not, in consequence of its attraction, allow any of its rays to arrive at us; it is therefore possible that the largest luminous bodies in the universe, may, through this cause, be invisible.
Pàgina 3 - According to the Principle of Relativity," he said, "the laws of physical phenomena must be the same for a 'fixed' observer as for an observer who has a uniform motion of translation relative to him : so that we have not, and cannot possibly have, any means of discerning whether we are, or are not, carried along in such a motion.
Pàgina 3 - I shall adduce will render this so obvious that there can hardly remain a doubt of the general motion of all the starry systems, and, consequently, of the solar one among the rest.
Pàgina 355 - The Production of the Elements Li, Be, B by Galactic Cosmic Rays in Space and its Relation with Stellar Observations', Astron.

Referències a aquest llibre

Sobre l'autor (2006)

Lang - Astrophysical Formulae Volume I

Astrophysical Formulae is a comprehensive, widely-used reference to the fundamental formulae employed in astronomy, astrophysics and general physics. All the basic formulae in a particular field are given, with references to both the original work and recent research papers. Where possible the formulae have been developed from basic principles. If you want to know something about a given area, or find the formula that you need or know might exist, the first step is to look for it in Astrophysical Formulae or its references, rather than searching through a library or journals.

Over the past two decades, Astrophysical Formulae has become a standard reference found on numerous individual bookshelves and in all libraries that deal with astronomy, astrophysics and physics. This third, enlarged and revised edition will be similarly used by current and future generations of students and scientists in these fields.

The new edition of Astrophysical Formulae has been divided into two books - Volume I. Radiation, Gas Processes and High Energy Astrophysics and Volume II. Space, Time, Matter and Cosmology. They together contain over 4000 formulae and 5000 references, more than doubling the number found in previous versions. Past editions have also been improved upon by collecting all the references together in one alphabetical bibliography, instead of listing by chapter, and numerous references have been added for papers published during the past three decades.

This Volume I. Radiation, Gas Processes and High Energy Astrophysics includes electromagnetic radiation, scattering and scintillation, atomic and molecular spectra with the various broadening and shifting effects, statistical mechanics and thermodynamics of gases, hydrodynamics and magnetohydrodynamics, and particle physics as far as it is applicable to astrophysics, including nucleosynthesis of the elements and energetic particles or radiation in the cosmos.

The material in Volume I has been updated with references to important review articles and books, and new formulae, data and references have been added for contemporary topics such as accretion, brown dwarfs, cosmic rays, spallation reactions, equations of state for degenerate gases, gamma ray bursts, gamma ray lines, interstellar gas and dust, molecular clouds, molecular masers, origin and abundance of the elements, particle acceleration by shock waves, star formation, supernovae explosions and remnants, supernova SN 1987A, and thermonuclear reactions. Entirely new sections include those on helioseismology, solar neutrinos, neutrino oscillations, neutrino emission from stellar collapse and supernovae, and energetic particles and radiation from solar flares.

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