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Radiatively-Driven Relativistic Accretion Disk Winds

机译:辐射驱动的相对论吸积盘风

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Wetheoreticallyexaminedrelativisticdiskwindsdrivenbydiskradiationfields.Forthepresentpurpose,wequantitativelycaluculatedthefullcomponentsofradiationfieldsproducedbyastandardaccretiondiskaroundSchwarzschildandextremeKerrblackholes,underthepseudo-Newtoniangravityandspecialrelativity.ThetypicalstrengthofradiationfieldsofdisksaroundtheSchwarzschildholereducesbyabout50%,whereasthataroundtheextremeKerrholeincreasesbyabouttentimes,ascomparedwiththeNewtoniancase.WefoundthatthewindiseasytoblowofffromthediskaroundtheKerrhole,althoughitbecomesdifficultfromthediskaroundtheSchwarzschildhole,aslongastheaccretionrateissubcritical.IntheextremeKerrcasethemaximumterminalspeedisabout$$0.5c$$forthecriticalaccretionrate.
机译:Wetheoreticallyexaminedrelativisticdiskwindsdrivenbydiskradiationfields.Forthepresentpurpose,wequantitativelycaluculatedthefullcomponentsofradiationfieldsproducedbyastandardaccretiondiskaroundSchwarzschildandextremeKerrblackholes,underthepseudo-Newtoniangravityandspecialrelativity.ThetypicalstrengthofradiationfieldsofdisksaroundtheSchwarzschildholereducesbyabout50%,whereasthataroundtheextremeKerrholeincreasesbyabouttentimes,ascomparedwiththeNewtoniancase.WefoundthatthewindiseasytoblowofffromthediskaroundtheKerrhole,althoughitbecomesdifficultfromthediskaroundtheSchwarzschildhole,aslongastheaccretionrateissubcritical.IntheextremeKerrcasethemaximumterminalspeedisabout $$ 0.5C $$ forthecriticalaccretionrate。

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