Abstract
TeV scale gravity scenario predicts that the black hole production dominates over all other interactions above the scale and that the Large Hadron Collider will be a black hole factory. Such higher-dimensional black holes mainly decay into the standard model fields via the Hawking radiation whose spectrum can be computed from the greybody factor. Here we complete the series of our work by showing the greybody factors and the resultant spectra for the brane-localized spinor and vector field emissions for arbitrary frequencies. Combining these results with the previous works, we determine the complete radiation spectra and the subsequent time evolution of the black hole. We find that, for a typical event, well more than half a black hole mass is emitted when the hole is still highly rotating, confirming our previous claim that it is important to take into account the angular momentum of black holes.
| Original language | English |
|---|---|
| Article number | 124022 |
| Journal | Physical Review D - Particles, Fields, Gravitation and Cosmology |
| Volume | 73 |
| Issue number | 12 |
| DOIs | |
| Publication status | Published - 2006 Jun 23 |
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All Science Journal Classification (ASJC) codes
- Nuclear and High Energy Physics
- Physics and Astronomy (miscellaneous)
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Rotating black holes at future colliders. III. Determination of black hole evolution. / Ida, Daisuke; Oda, Kin Ya; Park, Seong Chan.
In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 73, No. 12, 124022, 23.06.2006.Research output: Contribution to journal › Article
TY - JOUR
T1 - Rotating black holes at future colliders. III. Determination of black hole evolution
AU - Ida, Daisuke
AU - Oda, Kin Ya
AU - Park, Seong Chan
PY - 2006/6/23
Y1 - 2006/6/23
N2 - TeV scale gravity scenario predicts that the black hole production dominates over all other interactions above the scale and that the Large Hadron Collider will be a black hole factory. Such higher-dimensional black holes mainly decay into the standard model fields via the Hawking radiation whose spectrum can be computed from the greybody factor. Here we complete the series of our work by showing the greybody factors and the resultant spectra for the brane-localized spinor and vector field emissions for arbitrary frequencies. Combining these results with the previous works, we determine the complete radiation spectra and the subsequent time evolution of the black hole. We find that, for a typical event, well more than half a black hole mass is emitted when the hole is still highly rotating, confirming our previous claim that it is important to take into account the angular momentum of black holes.
AB - TeV scale gravity scenario predicts that the black hole production dominates over all other interactions above the scale and that the Large Hadron Collider will be a black hole factory. Such higher-dimensional black holes mainly decay into the standard model fields via the Hawking radiation whose spectrum can be computed from the greybody factor. Here we complete the series of our work by showing the greybody factors and the resultant spectra for the brane-localized spinor and vector field emissions for arbitrary frequencies. Combining these results with the previous works, we determine the complete radiation spectra and the subsequent time evolution of the black hole. We find that, for a typical event, well more than half a black hole mass is emitted when the hole is still highly rotating, confirming our previous claim that it is important to take into account the angular momentum of black holes.
UR - http://www.scopus.com/inward/record.url?scp=33745136160&partnerID=8YFLogxK
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U2 - 10.1103/PhysRevD.73.124022
DO - 10.1103/PhysRevD.73.124022
M3 - Article
AN - SCOPUS:33745136160
VL - 73
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
SN - 1550-7998
IS - 12
M1 - 124022
ER -