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SUMMARY:Polarization effects of algebraically special Maxwell field in the
  Kerr space-time
DTSTART;VALUE=DATE-TIME:20191224T103500Z
DTEND;VALUE=DATE-TIME:20191224T105500Z
DTSTAMP;VALUE=DATE-TIME:20260419T011242Z
UID:indico-contribution-132@indico.bitp.kiev.ua
DESCRIPTION:Speakers: Yurii Taistra (Pidstryhach Institute for Applied Pro
 blems of Mechanics and Mathematics National Academy of Sciences of Ukraine
 \, Lviv)\nFor obtaining polarization effects in the Kerr space-time we hav
 e used algebraically special approach for Maxwell equations [1].\nAs a con
 sequence\, in Kinnersley tetrad Maxwell field is described only by one ext
 remal component $\\varphi_2$\, and the Maxwell equations have closed-form 
 solution [2]:\n\n$\\varphi_2= C \\frac{e^{i\\omega (t-\\tilde{r}) + i m \\
 phi }}{\\sin\\theta(r- i a \\cos\\theta)} e^{-a\\omega\\cos\\theta} \\left
 (\\frac{1-\\cos\\theta}{\\sin\\theta}\\right)^m$\,\n\nwhere  $t>0$\, $ r_+
 \n\nhttps://indico.bitp.kiev.ua/event/4/contributions/132/
LOCATION:Bogolyubov Institute for Theoretical Physics of the National Acad
 emy of Sciences of Ukraine 322
URL:https://indico.bitp.kiev.ua/event/4/contributions/132/
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