Muutke küpsiste eelistusi

E-raamat: Astrophysics through Computation: With Mathematica(R) Support

(Rochester Institute of Technology, New York), (State University of New York, Geneseo)
  • Formaat: EPUB+DRM
  • Ilmumisaeg: 28-Jun-2013
  • Kirjastus: Cambridge University Press
  • Keel: eng
  • ISBN-13: 9781107272347
Teised raamatud teemal:
  • Formaat - EPUB+DRM
  • Hind: 70,38 €*
  • * hind on lõplik, st. muud allahindlused enam ei rakendu
  • Lisa ostukorvi
  • Lisa soovinimekirja
  • See e-raamat on mõeldud ainult isiklikuks kasutamiseks. E-raamatuid ei saa tagastada.
  • Formaat: EPUB+DRM
  • Ilmumisaeg: 28-Jun-2013
  • Kirjastus: Cambridge University Press
  • Keel: eng
  • ISBN-13: 9781107272347
Teised raamatud teemal:

DRM piirangud

  • Kopeerimine (copy/paste):

    ei ole lubatud

  • Printimine:

    ei ole lubatud

  • Kasutamine:

    Digitaalõiguste kaitse (DRM)
    Kirjastus on väljastanud selle e-raamatu krüpteeritud kujul, mis tähendab, et selle lugemiseks peate installeerima spetsiaalse tarkvara. Samuti peate looma endale  Adobe ID Rohkem infot siin. E-raamatut saab lugeda 1 kasutaja ning alla laadida kuni 6'de seadmesse (kõik autoriseeritud sama Adobe ID-ga).

    Vajalik tarkvara
    Mobiilsetes seadmetes (telefon või tahvelarvuti) lugemiseks peate installeerima selle tasuta rakenduse: PocketBook Reader (iOS / Android)

    PC või Mac seadmes lugemiseks peate installima Adobe Digital Editionsi (Seeon tasuta rakendus spetsiaalselt e-raamatute lugemiseks. Seda ei tohi segamini ajada Adober Reader'iga, mis tõenäoliselt on juba teie arvutisse installeeritud )

    Seda e-raamatut ei saa lugeda Amazon Kindle's. 

This new text surveys a series of fundamental problems in astrophysics, both analytically and computationally, for advanced students in physics and astrophysics. The contents are supported by more than 110 class-tested Mathematica® notebooks, allowing rigorous solutions to be explored in a visually engaging way. Topics covered include many classical and historically interesting problems, enabling students to appreciate the mathematical and scientific challenges that have been overcome in the subject's development. The text also shows the advantages and disadvantages of using analytical and computational methods. It will serve students, professionals and capable amateurs to master the quantitative details of modern astrophysics and the computational aspects of their research projects. Downloadable Mathematica® resources available at www.cambridge.org/koberlein.

Muu info

This new astrophysics text integrates analytical and computational methods to explore a broad range of topics in astrophysics.
Preface vii
1 Introduction
1(28)
1.1 Fundamental stellar properties
1(3)
1.2 Determination of stellar mass
4(3)
1.3 Kinetic theory
7(5)
1.4 Special relativity
12(9)
1.5 Image processing
21(8)
Exercises
27(2)
2 Stellar atmospheres
29(30)
2.1 Radiative transfer and the flow of photons through matter
29(5)
2.2 Formal solution of radiative transfer
34(6)
2.3 The gray-body approximation
40(8)
2.4 Continuous opacity in a real hydrogen star
48(3)
2.5 The case of spectrum lines
51(8)
Exercises
57(2)
3 Stellar interiors
59(45)
3.1 The hydrostatic model
59(4)
3.2 The polytropic star
63(7)
3.3 Stellar populations
70(8)
3.4 The virial theorem and stellar structure
78(9)
3.5 Fusion in the stellar core
87(9)
3.6 Beyond the polytropic model
96(8)
Exercises
102(2)
4 Extreme classical stars
104(39)
4.1 Atmospheres beyond local thermodynamic equilibrium
104(8)
4.2 Expanding atmospheres and the Sobolev method
112(12)
4.3 Properties of gas degeneracy
124(5)
4.4 White dwarfs
129(8)
4.5 Neutron stars
137(6)
Exercises
141(2)
5 General relativity and applications
143(43)
5.1 From special relativity to general relativity
143(5)
5.2 Mathematical toolbox
148(6)
5.3 Einstein's field equations
154(6)
5.4 Solving Einstein's equations
160(7)
5.5 Tests of general relativity
167(11)
5.6 Gravitational waves
178(8)
Exercises
185(1)
6 Binaries and clusters
186(34)
6.1 Variational mechanics
186(7)
6.2 The N-body problem
193(5)
6.3 The solar system
198(8)
6.4 The Trapezium system
206(7)
6.5 Chaotic systems
213(7)
Exercises
218(2)
7 Astrophysical plasmas
220(43)
7.1 Charges in cold plasmas
220(5)
7.2 Photons in cold plasmas
225(8)
7.3 Generalized magnetoionic radio wave propagation
233(5)
7.4 Pulsar signals as probes of the interstellar medium
238(6)
7.5 Warm plasmas
244(10)
7.6 Solar wind
254(9)
Exercises
260(3)
8 Galaxies
263(46)
8.1 The existence of dark matter
263(9)
8.2 Revisiting the Trapezium cluster
272(9)
8.3 The Henon Heiles equations
281(2)
8.4 The central black hole of the Milky Way
283(6)
8.5 Spiral density waves
289(5)
8.6 The interplay of gas and dust
294(12)
8.7 Galactic mergers
306(3)
Exercises
307(2)
9 Cosmic structures
309(48)
9.1 The Hubble law
309(5)
9.2 Quasars and radio galaxies
314(7)
9.3 Synchrotron radiation
321(5)
9.4 Distribution of galaxies
326(7)
9.5 Extragalactic bending of light
333(6)
9.6 The cosmic microwave background
339(7)
9.7 Cosmological models
346(11)
Exercises
354(3)
References 357(12)
Index 369
Brian Koberlein is Senior Lecturer in Physics and Astronomy at the Rochester Institute of Technology. David Meisel is Distinguished Professor of Physics and Astronomy at the State University of New York, Geneseo.