Black holes and time warps book
Black Holes and Time Warps - WikipediaThere are books we love and books we hate, and then there are books that irrevocably change our lives; for me, that book is "Black Holes and Time Warps" by Kip Thorne. I first heard the name Kip Thorne during my third year working on an undergraduate degree in physics, when my friend Dan gave me a beat-up paperback copy of Thorne's book, " Black Holes and Time Warps: Einstein's Outrageous Legacy. When Dan gave me the book we were both neck-deep in thermodynamics, stellar spectra, Brownian motion and all the things we had to cram into our heads to earn our degrees. It was a tough year, and a tough following year, and I think even then I had the sneaking suspicion that research wasn't where I belonged. I was feeling out of my place and out of my league among many of my peers, and I feared science would inevitably slip out of my life. But when I cracked open "Black Holes and Time Warps," the joy that had made me pursue science in the first place came back to me. It dives into what scientists know about power of gravity, the nature of space-time and the possibility of worm holes ; it touches on Einstein's theory of special relativity and some particle physics, among other things.
Black Holes & Time Warps: Einstein's Outrageous Legacy
This classic was first published in hardback in It is one of the best books written on the topic by one of the key players in the field. This book stands out for a number of reasons: 1 quality of the writing, 2 An excellent bibliography, and 3 very well done illustrations. I have lost count of the number of astronomy books published in the last years with poor quality photos or drawings. I wish Dr.
This book explains, among other thing, a very cool theory about using stable wormholes to create a time machine. Now if we could only make wormholes stable, manipulate them, and pass through them safely without radiation feedback An insider view of high energy physics by a hippie. This will explain black holes and quantum gravity. Don't let the publication date fool you. Unless you can do the math which this book blessedly Kip Thorne , Kip S.
It provides an illustrated overview of the history and development of black hole theory, from its roots in Newtonian mechanics until the early s. Over fourteen chapters, Thorne proceeds roughly chronologically, tracing first the crisis in Newtonian physics precipitated by the Michelson—Morley experiment , and the subsequent development of Einstein's theory of special relativity given mathematical rigor in the form of Minkowski space , and later Einstein's incorporation of gravity into the framework of general relativity. Black holes were quickly recognized as a feasible solution of Einstein's field equations , but were rejected as physically implausible by most physicists. Work by Subrahmanyan Chandrasekhar suggested that collapsing stars beyond a certain mass cannot be supported by degeneracy pressure , but this result was challenged by the more prestigious Arthur Stanley Eddington , and was not fully accepted for several decades. When the reality of objects which possess an event horizon finally achieved broad acceptance, the stage was set for a thorough investigation into the properties of such objects, yielding the surprising result that black holes have no hair —that is, that their properties are entirely determined by their mass, spin rate, and electrical charge. Proceeding separately from theoretical research into relativity, and with the refinement of radio astronomy , astrophysics began to produce unusual observations of extremely intense radio sources, which were apparently located outside of the Milky Way. In consultation with theoretical physicists, it became apparent that the only sensible explanation for these sources were extremely large black holes residing in the cores of galaxies, producing intense radiation as they fed and, in the case of quasars , blasting out incredibly powerful jets of material in opposite directions, heating the surrounding galactic gas until it glowed in radio frequencies.