000022273 001__ 22273
000022273 005__ 20140130004318.0
000022273 037__ $$9arXiv$$ahep-th/9908068$$chep-th
000022273 035__ $$9arXiv$$zoai:arXiv.org:hep-th/9908068
000022273 035__ $$9DESY$$zD99-14782
000022273 035__ $$9CERNKEY$$z0322600
000022273 035__ $$9SPIRESTeX$$zFilippov:1998jm
000022273 100__ $$aFilippov, A.T.$$uDubna, JINR
000022273 245__ $$aGlobal properties of exact solutions in integrable dilaton gravity models
000022273 246__ $$9arXiv$$aGlobal properties of exact solutions in integrable dilaton-gravity models.
000022273 269__ $$c1998-07
000022273 300__ $$a5
000022273 520__ $$aGlobal canonical transformations to free chiral fields are constructed for DG models minimally coupled to scalar fields. The boundary terms for such canonical transformations are shown to vanish in asymptotically static coordinates if there is no scalar field.
000022273 695__ $$2INSPIRE$$atalk: Dubna 1998/07/13
000022273 695__ $$2INSPIRE$$agravitation
000022273 695__ $$2INSPIRE$$adilaton
000022273 695__ $$2INSPIRE$$afield equations: solution
000022273 695__ $$2INSPIRE$$aasymptotic behavior
000022273 700__ $$aIvanov, V.G.$$uDubna, JINR
000022273 773__ $$tSubmitted to 11th International Conference on Problems of$$wC98/07/13.2
000022273 8564_ $$uhttp://alice.cern.ch/format/showfull?sysnb=0322600$$w0322600$$yCERNKEY
000022273 909CO $$ooai:jdsweb.jinr.ru:22273$$pglobal
000022273 961__ $$x1999-08-10
000022273 961__ $$c1999-12-15
000022273 970__ $$aSPIRES-4149483
000022273 980__ $$aarXiv
000022273 980__ $$aCiteable
000022273 980__ $$aCORE
000022273 999C5 $$rhep-th/9605008$$sMod.Phys.Lett.,A11,1691
000022273 999C5 $$rgr-qc/9612058$$sInt.J.Mod.Phys.,A12,13
000022273 999C5 $$rhep-th/9111056$$sPhys.Rev.,D45,1005
000022273 999C5 $$rhep-th/9704168$$sPhys.Rev.,D58,044010
000022273 999C5 $$rhep-th/9705145$$sMod.Phys.Lett.,A12,2345
000022273 999C5 $$rhep-th/9712194
000022273 999C5 $$sNucl.Phys.,B362,649
000022273 999C5 $$rgr-qc/9411070$$sInt.J.Mod.Phys.,D4,661
000022273 999C5 $$rgr-qc/9508062$$sInt.J.Mod.Phys.,D5,227
000022273 999C5 $$rgr-qc/9402031$$sInt.J.Mod.Phys.,A10,611
000022273 999C5 $$rgr-qc/9511081$$sClass.Quant.Grav.,13,2395
000022273 999C5 $$rgr-qc/9508020$$sClass.Quant.Grav.,13,965
000022273 999C5 $$rhep-th/9607226$$sClass.Quant.Grav.,14,1689
000022273 999C5 $$rhep-th/9505161$$sAnnals Phys.,245,408
000022273 999C5 $$rgr-qc/9608011$$sPhys.Rev.,D55,795
000022273 999C5 $$rhep-th/9802158$$sPhys.Lett.,B424,265