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Physics of Interstellar Dust [Hardback]

  • Formāts: Hardback, 584 pages, height x width: 234x156 mm, weight: 1124 g
  • Sērija : Series in Astronomy and Astrophysics
  • Izdošanas datums: 02-Dec-2002
  • Izdevniecība: Institute of Physics Publishing
  • ISBN-10: 0750308613
  • ISBN-13: 9780750308618
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  • Formāts: Hardback, 584 pages, height x width: 234x156 mm, weight: 1124 g
  • Sērija : Series in Astronomy and Astrophysics
  • Izdošanas datums: 02-Dec-2002
  • Izdevniecība: Institute of Physics Publishing
  • ISBN-10: 0750308613
  • ISBN-13: 9780750308618
Citas grāmatas par šo tēmu:
Interstellar dust grains catalyse chemical reactions, absorb, scatter, polarise and re-radiate starlight and constitute the building blocks for the formation of planets. Understanding this interstellar component is therefore of primary importance in many areas of astronomy & astrophysics. For example, observers need to understand how dust effects light passing through molecular clouds. Astrophysicists wish to comprehend how dust enables the collapse of clouds or how it determines the spectral behaviour of protostars, star forming regions or whole galaxies. This book gives a thorough theoretical description of the fundamental physics of interstellar dust: its composition, morphology, size distribution, dynamics, optical and thermal properties, alignment, polarisation, scattering, radiation and spectral features.

This encyclopedic book provides the basic physics towards understanding the solid matter in interstellar space. It includes all the necessary physics, including solid state physics, radiative transport, optical properties, thermodynamics, statistical mechanics and quantum mechanics. It then uses all of this basic physics in the specific case of dust grains in the interstellar medium.

Interstellar dust clouds catalyze simple chemical reactions, absorbs, scatters, polarizes and re-radiates starlight and forms the building blocks for planet and stellar formation. Understanding this interstellar medium is then of primary importance in many areas of astronomy & astrophysics. For example observers need to understand how it effects light passing through dust and molecular clouds, astrophysicists need to comprehend the formation and structure of dust clouds and how it collapses to form stars and planets.

Written in an accessible and descriptive manner, this will be essential supplementary reading for advanced undergraduate and graduate students taking courses on the interstellar medium and active researchers in need of a single source of well illustrated and detailed information.

Recenzijas

"It is by far the most comprehensive, detailed, and in depth work ever published on this subject. The book derives all of the relevant physics for interstellar dust from first principles. It includes all of the necessary physics of dust grains, including solid state physics, radiative transport, optical properties, thermodynamics, statistical mechanics and quantum mechanics. Its treatment of all of these subjects is detailed and precise. It then uses all of this basic physics in the specific case of dust grains in the interstellar medium. It represents the most complete volume on this subject and as such is a tremendous achievement. I am sure it will remain the standard text on this subject for many years to come." - Professor D. Ward-Thompson, Cardiff University, Wales

"It is the best book on cosmic dust..." - Professor A.V. Tutukov

"This is an encyclopaedic work, which will, I expect, prove a valuable reference for students and researchers in the field." - Professor B Draine

"The Physics of Interstellar Dust can be a valuable tool to anyone interested in the subject . . . In some ways, I view this book as containing almost all of physics applied to interstellar dust . . . This is a substantial book aimed at the specialized study of interstellar dust. I recommend that you definitely consider using this text if you have to teach a course about interstellar dust or want to do an independent study on the topic." - Edward L Wright, University of California in Physics Today, January 2004

"All of the material is presented clearly and concisely." - Tom Hartquist in A&G

Preface xix
The dielectric permeability
1(43)
Maxwell's equations
1(9)
Electric field and magnetic induction
1(1)
Electric polarization of the medium
2(1)
The dependence of the dielectric permeability on direction and frequency
3(1)
The physical meaning of the electric susceptibility X
4(2)
Magnetic polarization of the medium
6(1)
The magnetic susceptibility
7(1)
Dielectrics and metals
7(1)
Free charges and polarization charges
8(1)
The field equations
9(1)
Waves in a dielectric medium
10(5)
The wave equation
10(1)
The wavenumber
11(1)
The optical constant or refractive index
12(1)
Energy dissipation of a grain in a variable field
13(2)
The harmonic oscillator
15(7)
The Lorentz model
15(1)
Free oscillations
16(1)
The general solution to the oscillator equation
17(1)
Dissipation of energy in a forced oscillation
18(1)
Dissipation of energy in a free oscillation
19(1)
The plasma frequency
20(1)
Dispersion relation of the dielectric permeability
20(2)
The harmonic oscillator and light
22(10)
Attenuation and refraction of light
23(1)
Retarded potentials of a moving charge
24(2)
Emission of an harmonic oscillator
26(1)
Radiation of higher order
27(1)
Radiation damping
28(1)
The cross section of an harmonic oscillator
29(1)
The oscillator strength
30(1)
The natural linewidth
31(1)
Waves in a conducting medium
32(6)
The dielectric permeability of a conductor
33(1)
Conductivity and the Drude profile
34(2)
Electromagnetic waves in a plasma with a magnetic field
36(1)
Group velocity of electromagnetic waves in a plasma
37(1)
Polarization through orientation
38(6)
Polarization in a constant field
38(1)
Polarization in a time-variable field
39(1)
Relaxation after switching off the field
40(1)
The dielectric permeability in Debye relaxation
41(3)
How to evaluate grain cross sections
44(36)
Defining cross sections
44(3)
Cross section for scattering, absorption and extinction
44(2)
Cross section for radiation pressure
46(1)
Efficiencies, mass and volume coefficients
47(1)
The optical theorem
47(4)
The intensity of forward scattered light
47(3)
The refractive index of a dusty medium
50(1)
Mie theory for a sphere
51(6)
The generating function
52(1)
Separation of variables
52(2)
Series expansion of waves
54(1)
Expansion coefficients
54(2)
Scattered and absorbed power
56(1)
Absorption and scattering efficiencies
57(1)
Polarization and scattering
57(7)
The amplitude scattering matrix
57(1)
Angle-dependence of scattering
58(2)
The polarization ellipse
60(1)
Stokes parameters
61(1)
Stokes parameters of scattered light for a sphere
62(2)
The Kramers--Kronig relations
64(7)
Mathematical formulation of the relations
64(2)
The electric susceptibility and causality
66(1)
The Kramers--Kronig relation for the dielectric permeability
67(1)
Extension to metals
67(1)
Dispersion of the magnetic susceptibility
68(1)
Three corollaries of the KK relation
69(2)
Composite grains
71(9)
Effective medium theories
72(1)
Garnett's mixing rule
73(1)
The mixing rule of Bruggeman
74(1)
Composition of grains in protostellar cores
74(2)
How size, ice and porosity change the absorption coefficient
76(4)
Very small and very big particles
80(39)
Tiny spheres
80(7)
When is a particle in the Rayleigh limit?
80(1)
Efficiencies of small spheres from Mie theory
81(1)
A dielectric sphere in a constant electric field
82(2)
Scattering and absorption in the electrostatic approximation
84(1)
Polarization and angle-dependent scattering
85(1)
Small-size effects beyond Mie theory
86(1)
A small metallic sphere in a magnetic field
87(3)
Slowly varying field
87(2)
The magnetic polarizability
89(1)
The penetration depth
89(1)
Limiting values of the magnetic polarizability
90(1)
Tiny ellipsoids
90(9)
Elliptical coordinates
91(1)
An ellipsoid in a constant electric field
92(1)
Cross section and shape factor
93(2)
Randomly oriented ellipsoids
95(1)
Pancakes and cigars
95(2)
Rotation about the axis of greatest moment of inertia
97(2)
The fields inside a dielectric particle
99(4)
Internal field and depolarization field
99(1)
Depolarization field and the distribution of surface charges
100(1)
The local field at an atom
101(1)
The Clausius--Mossotti relation
101(2)
Very large particles
103(16)
Babinet's theorem
103(1)
Reflection and transmission at a plane surface
104(2)
Huygens' principle
106(3)
Fresnel zones and a check on Huygens' principle
109(2)
The reciprocity theorem
111(1)
Diffraction by a circular hole or a sphere
111(2)
Diffraction behind a half-plane
113(3)
Particles of small refractive index
116(1)
X-ray scattering
117(2)
Case studies of Mie calculus
119(26)
Efficiencies of bare spheres
119(8)
Pure scattering
119(1)
A weak absorber
120(2)
A strong absorber
122(1)
A metal sphere
123(1)
Efficiency versus cross section and volume coefficient
123(3)
The atmosphere of the Earth
126(1)
Scattering by bare spheres
127(5)
The scattering diagram
127(1)
The polarization of scattered light
128(3)
The intensity of scattered light in a reflection nebula
131(1)
Coated spheres
132(1)
Surface modes in small grains
133(3)
Efficiencies of idealized dielectrics and metals
136(9)
Dielectric sphere consisting of identical harmonic oscillators
136(2)
Dielectric sphere with Debye relaxation
138(1)
Magnetic and electric dipole absorption of small metal spheres
139(2)
Efficiencies for Drude profiles
141(1)
Elongated metallic particles
142(3)
Particle statistics
145(30)
Boltzmann statistics
145(6)
The probability of an arbitrary energy distribution
145(1)
The distribution of maximum probability
146(1)
Partition function and population of energy cells
147(2)
The mean energy of harmonic oscillators
149(1)
The Maxwellian velocity distribution
149(2)
Quantum statistics
151(9)
The unit cell h3 of the phase space
151(1)
Bosons and fermions
152(2)
Bose statistics
154(2)
Bose statistics for photons
156(1)
Fermi statistics
157(1)
Ionization equilibrium and the Saha equation
158(2)
Thermodynamics
160(10)
The ergodic hypothesis
160(2)
Definition of entropy and temperature
162(1)
The canonical distribution
163(1)
Thermodynamic relations for a gas
164(2)
Equilibrium conditions of the state functions
166(2)
Specific heat of a gas
168(1)
The work done by magnetization
168(1)
Susceptibility and specific heat of magnetic substances
169(1)
Blackbody radiation
170(5)
The Planck function
170(1)
Low- and high-frequency limit
171(1)
Wien's displacement law and the Stefan--Boltzmann law
172(1)
The Planck function and harmonic oscillators
173(2)
The radiative transition probability
175(26)
A charged particle in an electromagnetic field
175(6)
The classical Hamiltonian
175(1)
The Hamiltonian of an electron in an electromagnetic field
176(1)
The Hamilton operator in quantum mechanics
177(2)
The dipole moment in quantum mechanics
179(1)
The quantized harmonic oscillator
179(2)
Small perturbations
181(2)
The perturbation energy
181(1)
The transition probability
181(1)
Transition probability for a time-variable perturbation
182(1)
The Einstein coefficients A and B
183(9)
Induced and spontaneous transitions
183(3)
Selection rules and polarization rules
186(1)
Quantization of the electromagnetic field
186(2)
Quantum-mechanical derivation of A and B
188(4)
Potential wells and tunneling
192(9)
Wavefunction of a particle in a constant potential
192(1)
Potential walls and Fermi energy
192(2)
Rectangular potential barriers
194(4)
The double potential well
198(3)
Structure and composition of dust
201(38)
Crystal structure
201(6)
Translational symmetry
201(2)
Lattice types
203(4)
The reciprocal lattice
207(1)
Binding in crystals
207(7)
Covalent bonding
208(1)
Ionic bonding
209(2)
Metals
211(2)
van der Waals forces and hydrogen bridges
213(1)
Reddening by interstellar grains
214(10)
Stellar photometry
214(2)
The interstellar extinction curve
216(3)
Two-color diagrams
219(1)
Spectral indices
220(2)
The mass absorption coefficient
222(2)
Carbonaceous grains and silicate grains
224(10)
Origin of the two major dust constituents
224(1)
The bonding in carbon
225(2)
Carbon compounds
227(5)
Silicates
232(1)
A standard set of optical constants
233(1)
Grain sizes and optical constants
234(5)
The size distribution
234(2)
Collisional fragmentation
236(3)
Dust radiation
239(36)
Kirchhoff's law
239(4)
The emissivity of dust
239(1)
Thermal emission of grains
240(1)
Absorption and emission in thermal equilibrium
241(1)
Equipartition of energy
242(1)
The temperature of big grains
243(8)
The energy equation
243(1)
Approximate absorption efficiency at infrared wavelengths
243(2)
Temperature estimates
245(2)
Relation between grain size and grain temperature
247(1)
Temperature of dust grains near a star
248(1)
Dust temperatures from observations
249(2)
The emission spectrum of big grains
251(3)
Constant temperature and low optical depth
251(2)
Constant temperature and arbitrary optical depth
253(1)
Calorific properties of solids
254(8)
Normal coordinates
254(2)
Internal energy of a grain
256(1)
Standing waves in a crystal
257(1)
The density of vibrational modes in a crystal
258(1)
Specific heat
259(2)
Two-dimensional lattices
261(1)
Temperature fluctuations of very small grains
262(6)
The probability density P(T)
263(1)
The transition matrix
263(2)
Practical considerations
265(1)
The stochastic time evolution of grain temperature
266(2)
The emission spectrum of very small grains
268(7)
Small and moderate fluctuations
268(2)
Strong fluctuations
270(2)
Temperature fluctuations and flux ratios
272(3)
Dust and its environment
275(44)
Grain surfaces
275(10)
Gas accretion on grains
275(1)
Physical adsorption and chemisorption
276(3)
The sticking probability
279(2)
Thermal hopping, evaporation and reactions with activation barrier
281(2)
Tunneling between surface sites
283(1)
Scanning time
284(1)
Grain charge
285(4)
Charge equilibrium in the absence of a UV radiation field
285(1)
The photoelectric effect
286(3)
Grain motion
289(9)
Random walk
289(1)
The drag on a grain subjected to a constant outer force
289(3)
Brownian motion of a grain
292(1)
The disorder time
293(2)
Laminar and turbulent friction
295(1)
A falling rain drop
296(1)
The Poynting--Robertson effect
297(1)
Grain destruction
298(3)
Mass balance in the Milky Way
298(1)
Destruction processes
299(2)
Grain formation
301(18)
Evaporation temperature of dust
301(3)
Vapor pressure of small grains
304(1)
Critical saturation
305(2)
Equations for time-dependent homogeneous nucleation
307(1)
Equilibrium distribution and steady-state nucleation
308(3)
Solutions to time-dependent homogeneous nucleation
311(5)
Similarity relations
316(3)
Polarization
319(28)
Efficiency of infinite cylinders
319(8)
Normal incidence and picket fence alignment
319(3)
Oblique incidence
322(1)
Rotating cylinders
322(3)
Absorption efficiency as a function of wavelength
325(2)
Linear polarization through extinction
327(12)
Effective optical depth and degree of polarization p(λ)
327(2)
The Serkowski curve
329(2)
Polarization p(λ) of infinite cylinders
331(3)
Polarization p(λ) of ellipsoids in the Rayleigh limit
334(3)
Polarization p(λ) of spheroids at optical wavelengths
337(1)
Polarization and reddening
338(1)
Polarized emission
339(3)
The wavelength dependence of polarized emission for cylinders
340(1)
Infrared emission of spheroids
340(1)
Polarized emission versus polarized extinction
341(1)
Circular polarization
342(5)
The phase shift induced by grains
343(1)
The wavelength dependence of circular polarization
344(3)
Grain alignment
347(30)
Grain rotation
347(8)
Euler's equations for a rotating body
347(2)
Symmetric tops
349(2)
Atomic magnet in a magnetic field
351(1)
Rotational Brownian motion
351(2)
Suprathermal rotation
353(2)
Magnetic dissipation
355(9)
Diamagnetism
355(1)
Paramagnetism
355(2)
Ferromagnetism
357(1)
The magnetization of iron above and below the Curie point
358(1)
Paramagnetic dissipation: spin--spin and spin--lattice relaxation
359(1)
The magnetic susceptibility for spin--lattice relaxation
360(2)
The magnetic susceptibility in spin--spin relaxation
362(2)
Magnetic alignment
364(9)
A rotating dipole in a magnetic field
365(2)
Timescales for alignment and disorder
367(1)
Super-paramagnetism
368(1)
Ferromagnetic relaxation
369(2)
Alignment of angular momentum with the axis of greatest inertia
371(1)
Mechanical and magnetic damping
372(1)
Non-magnetic alignment
373(4)
Gas streaming
373(2)
Anisotropic illumination
375(2)
PAHs and spectral features of dust
377(19)
Thermodynamics of PAHs
377(7)
What are PAHs?
377(1)
Microcanonic emission of PAHs
378(1)
The vibrational modes of anthracene
379(2)
Microcanonic versus thermal level population
381(1)
Does an ensemble of PAHs have a temperature?
382(2)
PAH emission
384(4)
Photoexcitation of PAHs
384(1)
Cutoff wavelength for electronic excitation
385(1)
Photo-destruction and ionization
386(1)
Cross sections and line profiles of PAHs
387(1)
Big grains and ices
388(2)
The silicate features and the band at 3.4 μm
389(1)
Icy grain mantles
389(1)
An overall dust model
390(6)
The three dust components
392(3)
Extinction coefficient in the diffuse medium
395(1)
Extinction coefficient in protostellar cores
395(1)
Radiative transport
396(29)
Basic transfer relations
396(6)
Radiative intensity and flux
396(2)
The transfer equation and its formal solution
398(2)
The brightness temperature
400(1)
The main-beam-brightness temperature of a telescope
401(1)
Spherical clouds
402(7)
Moment equations for spheres
403(1)
Frequency averages
404(1)
Differential equations for the intensity
405(2)
Integral equations for the intensity
407(1)
Practical hints
407(2)
Passive disks
409(6)
Radiative transfer in a plane parallel layer
409(5)
The grazing angle in an inflated disk
414(1)
Galactic nuclei
415(3)
Hot spots in a spherical stellar cluster
415(1)
Low and high luminosity stars
416(2)
Line radiation
418(7)
Absorption coefficient and absorption profile
418(1)
The excitation temperature of a line
419(1)
Radiative transfer in lines
420(5)
Diffuse matter in the Milky Way
425(36)
Overview of the Milky Way
425(2)
Global parameters
425(1)
The relevance of dust
426(1)
Molecular clouds
427(11)
The CO molecule
428(3)
Population of levels in CO
431(4)
Molecular hydrogen
435(1)
Formation of molecular hydrogen on dust surfaces
435(3)
Clouds of atomic hydrogen
438(10)
General properties of the diffuse gas
438(1)
The 21 cm line of atomic hydrogen
439(1)
How the hyperfine levels of atomic hydrogen are excited
440(3)
Gas density and temperature from the 21 cm line
443(1)
The deuterium hyperfine line
444(2)
Electron density and magnetic field in the diffuse gas
446(2)
HII regions
448(9)
Ionization and recombination
448(2)
Dust--free HII regions
450(3)
Dusty HII regions
453(2)
Bremsstrahlung
455(1)
Recombination lines
456(1)
Mass estimates of interstellar clouds
457(4)
From optically thin CO lines
457(1)
From the CO luminosity
458(1)
From dust emission
459(2)
Stars and their formation
461(44)
Stars on and beyond the main sequence
461(10)
Nuclear burning and the creation of elements
461(2)
The binding energy of an atomic nucleus
463(2)
Hydrogen burning
465(2)
The 3α process
467(2)
Lifetime and luminosity of stars
469(1)
The initial mass function
470(1)
Clouds near gravitational equilibrium
471(15)
Virialized clouds
471(3)
Isothermal cloud in pressure equilibrium
474(1)
Structure and stability of Ebert--Bonnor spheres
475(4)
Free-fall of a gas ball
479(1)
The critical mass for gravitational instability
480(2)
Implications of the Jeans criterion
482(2)
Magnetic fields and ambipolar diffusion
484(2)
Gravitational collapse
486(8)
The presolar nebula
486(1)
Hydrodynamic collapse simulations
487(4)
Similarity solutions of collapse
491(3)
Disks
494(11)
Viscous laminar flows
494(3)
Dynamical equations of the thin accretion disk
497(1)
The Kepler disk
498(1)
Why a star accretes from a disk
499(2)
The stationary accretion disk
501(1)
The α-disk
501(2)
Disk heating by viscosity
503(2)
Emission from young stars
505(34)
The earliest stages of star formation
505(3)
Globules
505(1)
Isothermal gravitationally-bound clumps
506(2)
The collapse phase
508(10)
The density structure of a protostar
508(5)
Dust emission from a solar-type protostar
513(2)
Kinematics of protostellar collapse
515(3)
Accretion disks
518(6)
A flat blackbody disk
518(3)
A flat non-blackbody disk
521(1)
Radiative transfer in an inflated disk
522(2)
Reflection nebulae
524(2)
Cold and warm dust in galaxies
526(5)
Starburst nuclei
531(8)
Repetitive bursts of star formation
531(4)
Dust emission from starburst nuclei
535(4)
Appendix A Mathematical formulae 539(6)
Appendix B List of symbols 545(4)
References 549(3)
Index 552
Endrik Krügel Max-Planck-Institut für Radioastronomie, Bonn, Germany