000 | 02762nam a22004095a 4500 | ||
---|---|---|---|
001 | 93-091109 | ||
003 | CH-001817-3 | ||
005 | 20170613140746.0 | ||
006 | a fot ||| 0| | ||
007 | cr nn mmmmamaa | ||
008 | 091109e20090110sz fot ||| 0|eng d | ||
020 | _a9783037195680 | ||
024 | 7 | 0 |
_a10.4171/068 _2doi |
040 | _ach0018173 | ||
072 | 7 |
_aPHRD _2bicssc |
|
084 |
_a83-xx _a35-xx _a58-xx _2msc |
||
100 | 1 |
_aChristodoulou, Demetrios, _eauthor. |
|
245 | 1 | 0 |
_aThe Formation of Black Holes in General Relativity _h[electronic resource] / _cDemetrios Christodoulou |
260 | 3 |
_aZuerich, Switzerland : _bEuropean Mathematical Society Publishing House, _c2009 |
|
264 | 1 |
_aZuerich, Switzerland : _bEuropean Mathematical Society Publishing House, _c2009 |
|
300 | _a1 online resource (598 pages) | ||
336 |
_atext _btxt _2rdacontent |
||
337 |
_acomputer _bc _2rdamedia |
||
338 |
_aonline resource _bcr _2rdacarrier |
||
347 |
_atext file _bPDF _2rda |
||
490 | 0 | _aEMS Monographs in Mathematics (EMM) | |
506 | 1 |
_aRestricted to subscribers: _uhttp://www.ems-ph.org/ebooks.php |
|
520 | _aIn 1965 Penrose introduced the fundamental concept of a trapped surface, on the basis of which he proved a theorem which asserts that a spacetime containing such a surface must come to an end. The presence of a trapped surface implies, moreover, that there is a region of spacetime, the black hole, which is inaccessible to observation from infinity. A major challenge since that time has been to find out how trapped surfaces actually form, by analyzing the dynamics of gravitational collapse. The present monograph achieves this aim by establishing the formation of trapped surfaces in pure general relativity through the focusing of gravitational waves. The theorems proved in the present monograph constitute the first foray into the long-time dynamics of general relativity in the large, that is, when the initial data are no longer confined to a suitable neighborhood of trivial data. The main new method, the short pulse method, applies to general systems of Euler–Lagrange equations of hyperbolic type, and provides the means to tackle problems which have hitherto seemed unapproachable. This monograph will be of interest to people working in general relativity, geometric analysis, and partial differential equations. | ||
650 | 0 | 7 |
_aGeneral relativity _2bicssc |
650 | 0 | 7 |
_aRelativity and gravitational theory _2msc |
650 | 0 | 7 |
_aPartial differential equations _2msc |
650 | 0 | 7 |
_aGlobal analysis, analysis on manifolds _2msc |
700 | 1 |
_aChristodoulou, Demetrios, _eauthor. |
|
856 | 4 | 0 | _uhttps://doi.org/10.4171/068 |
856 | 4 | 2 |
_3cover image _uhttp://www.ems-ph.org/img/books/christodoulou3_mini.jpg |
942 |
_2EBK13772 _cEBK |
||
999 |
_c50396 _d50396 |