https://doi.org/10.1140/epjc/s10052-019-7452-6
Regular Article - Theoretical Physics
Hawking emission of charged particles from an electrically charged spherical black hole with scalar hair
IISER Kolkata, Mohanpur Campus, Nadia, Mohanpur, 741246, India
* e-mail: ac13ip001@iiserkol.ac.in
Received:
27
August
2019
Accepted:
31
October
2019
Published online:
15
November
2019
A static spherically symmetric black hole usually turns out to be either a Schwarzschild black hole or a Reissner-Nordström black hole. This result was summarised by Ruffini and Wheeler as the so-called no hair conjecture which states that for a spherically symmetric black hole only the information about mass (M) and electric charge (e) of the black hole is available for an external observer. In this work, we calculate the emission rate of charged particles from an asymptotically flat charged spherically symmetric black hole endowed with a scalar hair using a semi-classical tunneling formalism. We observe that the total entropy of the black hole contains an energy-dependent part due to the scalar charge. The upper bound on the charge-mass ratio of the emitted particles is also observed to decrease with the scalar charge as well.
© The Author(s), 2019
