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pro vyhledávání: '"polarization: vector"'
Autor:
Grimms, Caleb J., Nevels, Robert D.
In this paper the finite-difference time-domain general vector auxiliary differential equation method [Greene, J. H. and A. Taflove, Opt. Express 14, 8305 (2006)], nonlinear polarization vector, the nonlinear electric dipole moment per unit volume, i
Externí odkaz:
http://arxiv.org/abs/2410.16622
This report presents the results of optical polarimetric observations carried out with 6-m and 1-m telescopes at SAO RAS. The study of the blazar S5 0716+714 radiation showed the presence of a period of the variability of brightness and polarization
Externí odkaz:
http://arxiv.org/abs/2309.14299
Publikováno v:
Proceedings of the International Astronomical Union. Dec2022, Vol. 17 Issue S375, p66-70. 5p.
Akademický článek
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For a general $H_b\to H_c\tau\bar\nu_\tau$ decay we analyze the role of the $\tau$ polarization vector ${\cal P}^\mu$ in the context of lepton flavor universality violation studies. We use a general phenomenological approach that includes, in additio
Externí odkaz:
http://arxiv.org/abs/2103.01857
Autor:
Shablovinskaya, E., Afanasiev, V.
Publikováno v:
Contributions of the Astronomical Observatory Skalnate Pleso, 2020, vol. 50, no. 1, p. 341-349
The bright radio source S5 0716+714, which is usually classified as a BL Lac object, is one of the most intensively studied blazar. S5 0716+714 demonstrates extremely peculiar properties, such as the shortest time-scale of optical and polarimetric va
Externí odkaz:
http://arxiv.org/abs/2003.12822
Publikováno v:
In Wave Motion December 2018 83:202-213
The bright radio source S5 0716+714, that is usually classified as BL Lac object, is one of the most intensively studied. S5 0716+714 demonstrates extremely peculiar properties such as the shortest time-scale of optical and polarimetric variations ob
Externí odkaz:
http://arxiv.org/abs/1810.07594
Autor:
Ghosh, Tanay, Sen, Asoke K.
In the present work, rotation of the polarization vector of an electromagnetic wave is extensively calculated for a rotating observer, who can also be considered as a non-inertial accelerated observer. The rotation of the polarization vector calculat
Externí odkaz:
http://arxiv.org/abs/1806.06130
Autor:
Imazawa, Ryo1 imazawa@astro.hiroshima-u.ac.jp, Sasada, Mahito2,3, Hazama, Natsuko1, Fukazawa, Yasushi1,4, Nakaoka, Tatsuya3, Akitaya, Hiroshi5, Kawabata, Koji S.3, Bohn, Thomas3, Gangopadhyay, Anjasha3
Publikováno v:
Proceedings of the International Astronomical Union. Dec2022, Vol. 17 Issue S375, p61-65. 5p.