Speaker
Mr
Abdullo Hakimov
(Ulugh Beg Astronomical Institute of the Uzbek Academy of Scienses)
Description
The exterior electromagnetic fields of slowly rotating relativistic magnetized star in the braneworld are studied in detail. The dependence of the electromagnetic energy losses of the rotating magnetized star from the brane tension is also calculated and has been combined with the astrophysical data on pulsar period slow down in order to get constraints on the brane parameter. We have found the upper limit for the brane parameter as $Q ≲ 3\times 10^{11}$cm$^2$.
Primary author
Mr
Abdullo Hakimov
(Ulugh Beg Astronomical Institute of the Uzbek Academy of Scienses)
