My Account Log in

1 option

Dynamics and evolution of galactic nuclei / David Merritt.

De Gruyter Princeton University Press eBook-Package Backlist 2000-2013 Available online

View online
Format:
Book
Author/Creator:
Merritt, David, 1955 November 16- author.
Series:
Princeton series in astrophysics ; Volume 23.
Princeton Series in Astrophysics ; Volume 23
Language:
English
Subjects (All):
Active galactic nuclei.
Galactic nuclei--Evolution.
Galactic nuclei.
Galaxies--Evolution.
Galaxies.
Physical Description:
1 online resource (567 pages)
Place of Publication:
Princeton, New Jersey : Princeton University Press, [2013]
Summary:
Deep within galaxies like the Milky Way, astronomers have found a fascinating legacy of Einstein's general theory of relativity: supermassive black holes. Connected to the evolution of the galaxies that contain these black holes, galactic nuclei are the sites of uniquely energetic events, including quasars, stellar tidal disruptions, and the generation of gravitational waves. This textbook is the first comprehensive introduction to dynamical processes occurring in the vicinity of supermassive black holes in their galactic environment. Filling a critical gap, it is an authoritative resource for astrophysics and physics graduate students, and researchers focusing on galactic nuclei, the astrophysics of massive black holes, galactic dynamics, and gravitational wave detection. It is an ideal text for an advanced graduate-level course on galactic nuclei and as supplementary reading in graduate-level courses on high-energy astrophysics and galactic dynamics. David Merritt summarizes the theoretical work of the last three decades on the evolution of galactic nuclei, the formation of massive black holes, and the interaction between black holes and stars. He explores in depth such important topics as observations of galactic nuclei, dynamical models, weighing black holes, motion near supermassive black holes, evolution of nuclei due to gravitational encounters, loss cone theory, and binary supermassive black holes. Self-contained and up-to-date, the textbook includes a summary of the current literature and previously unpublished work by the author. For researchers working on active galactic nuclei, galaxy evolution, and the generation of gravitational waves, this book will be an essential resource.
Contents:
Cover
Title
Copyright
Dedication
Contents
Preface
Chapter 1 INTRODUCTION AND HISTORICAL OVERVIEW
Chapter 2 OBSERVATIONS OF GALACTIC NUCLEI AND SUPERMASSIVE BLACK HOLES
2.1 Structure of galaxies and galactic nuclei
2.2 Techniques for weighing black holes
2.3 Supermassive black holes in the Local Group
2.4 Phenomenology
2.5 Evidence for intermediate-mass black holes
2.6 Evidence for binary and multiple supermassive black holes
2.7 Gravitational waves
Chapter 3 COLLISIONLESS EQUILIBRIA
3.1 Orbits, integrals, and steady states
3.2 Spherical nuclei
3.3 The adiabatic growth model
3.4 Axisymmetric nuclei
3.5 Triaxial nuclei
Chapter 4 MOTION NEAR SUPERMASSIVE BLACK HOLES
4.1 Keplerian orbits
4.2 Perturbed orbits
4.3 The post-Newtonian approximation
4.4 Newtonian perturbations
4.5 Relativistic orbits
4.6 Capture
4.7 Relativistic motion in the presence of a distributed mass
4.8 Motion in the presence of a second massive body
4.9 Stellar motions at the center of the Milky Way
Chapter 5 THEORY OF GRAVITATIONAL ENCOUNTERS
5.1 Basic concepts and time of relaxation
5.2 Diffusion coefficients
5.3 Fokker-Planck equation
5.4 Gravitational Brownian motion
5.5 Orbit-averaged Fokker-Planck equation
5.6 Gravitational encounters near a supermassive black hole
5.7 Encounters with a spinning supermassive black hole
Chapter 6 LOSS-CONE DYNAMICS
6.1 Spherical symmetry
6.2 Nonspherical nuclei
6.3 Binary and hypervelocity stars
6.4 Relativistic loss cones and extreme-mass-ratio inspirals
Chapter 7 COLLISIONAL EVOLUTION OF NUCLEI
7.1 Evolution of the stellar distribution around a supermassive black hole
7.2 Cusp (re)generation
7.3 Black-hole-driven expansion
7.4 Massive perturbers
7.5 Evolution of nuclei lacking massive black holes.
Chapter 8 BINARY AND MULTIPLE SUPERMASSIVE BLACK HOLES
8.1 Interaction of a massive binary with field stars
8.2 Massive binary at the center of a galaxy: I. Early evolution
8.3 Massive binary at the center of a galaxy: II. Late evolution
8.4 Interaction of binary supermassive black holes with gas
8.5 Simulations of galaxy mergers
8.6 Dynamics of intermediate-mass black holes
8.7 Triple supermassive black holes and the final-parsec problem
Suggestions for Further Reading
References
Index.
Notes:
Description based on print version record.
ISBN:
9781400846122
1400846129
OCLC:
958573669

The Penn Libraries is committed to describing library materials using current, accurate, and responsible language. If you discover outdated or inaccurate language, please fill out this feedback form to report it and suggest alternative language.

My Account

Shelf Request an item Bookmarks Fines and fees Settings

Guides

Using the Library Catalog Using Articles+ Library Account