000 01797nam a22004455i 4500
001 978-3-540-37146-5
003 DE-He213
005 20190213151411.0
007 cr nn 008mamaa
008 121227s1972 gw | s |||| 0|eng d
020 _a9783540371465
_9978-3-540-37146-5
024 7 _a10.1007/3-540-05741-2
_2doi
050 4 _aQC1-75
072 7 _aPH
_2bicssc
072 7 _aSCI055000
_2bisacsh
072 7 _aPH
_2thema
082 0 4 _a530
_223
100 1 _aRyan, Michael.
_eauthor.
_4aut
_4http://id.loc.gov/vocabulary/relators/aut
245 1 0 _aHamiltonian Cosmology
_h[electronic resource] /
_cby Michael Ryan.
264 1 _aBerlin, Heidelberg :
_bSpringer Berlin Heidelberg,
_c1972.
300 _aVII, 172 p. 1 illus.
_bonline resource.
336 _atext
_btxt
_2rdacontent
337 _acomputer
_bc
_2rdamedia
338 _aonline resource
_bcr
_2rdacarrier
347 _atext file
_bPDF
_2rda
490 1 _aLecture Notes in Physics,
_x0075-8450 ;
_v13
505 0 _aThe ADM formalism applied to homogeneous cosmologies -- The Hamiltonian formalism: Simple examples, their classical and quantum behavior -- The Hamiltonian formulation applied to more complex systems -- Applications to Bianchi-type universes -- Superspace -- Quantization.
650 0 _aPhysics.
650 1 4 _aPhysics, general.
_0http://scigraph.springernature.com/things/product-market-codes/P00002
710 2 _aSpringerLink (Online service)
773 0 _tSpringer eBooks
776 0 8 _iPrinted edition:
_z9783540057413
776 0 8 _iPrinted edition:
_z9783662164280
830 0 _aLecture Notes in Physics,
_x0075-8450 ;
_v13
856 4 0 _uhttps://doi.org/10.1007/3-540-05741-2
912 _aZDB-2-PHA
912 _aZDB-2-LNP
912 _aZDB-2-BAE
999 _c10546
_d10546