1.

Record Nr.

UNISA996466812803316

Titolo

Astrophysical Black Holes [[electronic resource] /] / edited by Francesco Haardt, Vittorio Gorini, Ugo Moschella, Aldo Treves, Monica Colpi

Pubbl/distr/stampa

Cham : , : Springer International Publishing : , : Imprint : Springer, , 2016

ISBN

3-319-19416-X

Edizione

[1st ed. 2016.]

Descrizione fisica

1 online resource (XII, 314 p. 107 illus., 88 illus. in color.)

Collana

Lecture Notes in Physics, , 0075-8450 ; ; 905

Disciplina

523.8875

Soggetti

Astrophysics

Gravitation

Astrophysics and Astroparticles

Classical and Quantum Gravitation, Relativity Theory

Lingua di pubblicazione

Inglese

Formato

Materiale a stampa

Livello bibliografico

Monografia

Note generali

Bibliographic Level Mode of Issuance: Monograph

Nota di contenuto

Preface -- An introduction to astrophysical black holes and their dynamical Production -- Warp propagation in astrophysical discs -- The balance of power: accretion and feedback in stellar mass black Holes --  Observing Supermassive Black Holes across cosmic time: from phenomenology to physics -- Orbital Motion in Galactic Nuclei -- Star Formation and Dynamics in the Galactic Centre -- The effective-one-body approach to the general relativistic two body problem -- Index.

Sommario/riassunto

Based on graduate school lectures in contemporary relativity and gravitational physics, this book gives a complete and unified picture of the present status of theoretical and observational properties of astrophysical black holes. The chapters are written by internationally recognized specialists. They cover general theoretical aspects of black hole astrophysics, the theory of accretion and ejection of gas and jets, stellar-sized black holes observed in the Milky Way, the formation and evolution of supermassive black holes in galactic centers and quasars as well as their influence on the dynamics in galactic nuclei. The final chapter addresses analytical relativity of black holes supporting theoretical understanding of the coalescence of black holes as well as being of great relevance in identifying gravitational wave signals. With



its introductory chapters the book is aimed at advanced graduate and post-graduate students, but it will also be useful for specialists.