Black Hole Astrophysics
• reviews our current knowledge of cosmic black holes and how they generate the most powerful observed pheonomena in the Universe;
• highlights the latest, most up-to-date theories and discoveries in this very active area of astrophysical research;
• demonstrates why we believe that black holes are responsible for important phenomena such as quasars, microquasars and gammaray bursts;
• explains to the reader the nature of the violent and spectacular outfl ows (winds and jets) generated by black hole accretion.
David Meier is a Senior Research Scientist and supervisor of the Evolution of Galaxies Group at Caltech's Jet Propulsion Laboratory in Pasadena, CA. David had an early career doing research in genetics at Washington University School of Medicine and in solid state physics at the University of Missouri - Rolla (UMR), before achieving his goal of research in astrophysics. He was educated in physics at UMR (BS 1971; MS 1973) and in astrophysics at The University of Texas at Austin (MA 1975; PhD 1977), working there under D. Schramm, B. Tinsley, and J.C. Wheeler on astrophysical jet production, galaxy formation, and winds from accretion disks around black holes. In 1976, with Tinsley, he predicted the existence of primeval Lyman break galaxies, which since have been discovered and found to have many of their expected properties. At Caltech and JPL David has been an integral part of a number of projects and missions involving observations of galaxies and black hole systems, including very long baseline radio interferometry (VLBI) in the southern hemisphere, VLBI using a space-based antenna (which created a telescope three times the size of the earth), and the space interferometer mission SIM. He also spent several years working on the US government's “star wars” project and was the group leader for parallel computing applications in that effort. While much of his recent work has been theoretical investigations of accretion inflows and outflows from black holes systems, David also enjoys occasional observational studies, using some of the satellites and telescopes on which he has worked. He also greatly enjoys his three grandsons, with a fourth soon to arrive.
What is the nature of space and time? How do we fit within the universe? How does the universe fit within us? There’s no better guide through these mind-expanding questions than acclaimed astrophysicist and best-selling author Neil deGrasse Tyson.
But today, few of us have time to contemplate the cosmos. So Tyson brings the universe down to Earth succinctly and clearly, with sparkling wit, in tasty chapters consumable anytime and anywhere in your busy day.
While you wait for your morning coffee to brew, for the bus, the train, or a plane to arrive, Astrophysics for People in a Hurry will reveal just what you need to be fluent and ready for the next cosmic headlines: from the Big Bang to black holes, from quarks to quantum mechanics, and from the search for planets to the search for life in the universe.
This text covers a broad range of topics for a graduate-level class in a physics department where students' available credit hours for astrophysics classes are limited. The sections cover galactic structure, external galaxies, galaxy clustering, active galaxies, general relativity and cosmology.
With an emphasis on geometric interpretation, this masterful and comprehensive book introduces the theory of relativity; describes physical applications, from stars to black holes and gravitational waves; and portrays the field’s frontiers. The book also offers a unique, alternating, two-track pathway through the subject. Material focusing on basic physical ideas is designated as Track 1 and formulates an appropriate one-semester graduate-level course. The remaining Track 2 material provides a wealth of advanced topics instructors can draw on for a two-semester course, with Track 1 sections serving as prerequisites.
This must-have reference for students and scholars of relativity includes a new preface by David Kaiser, reflecting on the history of the book’s publication and reception, and a new introduction by Charles Misner and Kip Thorne, discussing exciting developments in the field since the book’s original publication.
The book teaches students to:Grasp the laws of physics in flat and curved spacetimePredict orders of magnitudeCalculate using the principal tools of modern geometryUnderstand Einstein's geometric framework for physicsExplore applications, including neutron stars, Schwarzschild and Kerr black holes, gravitational collapse, gravitational waves, cosmology, and so much more