Rotating black holes at future colliders. III. Determination of black hole evolution

Daisuke Ida, Kin Ya Oda, Seong Chan Park

Research output: Contribution to journalArticle

66 Citations (Scopus)

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 languageEnglish
Article number124022
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume73
Issue number12
DOIs
Publication statusPublished - 2006 Jun 23

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radiation spectra
industrial plants
field emission
angular momentum
gravitation
decay
interactions

All Science Journal Classification (ASJC) codes

  • Nuclear and High Energy Physics
  • Physics and Astronomy (miscellaneous)

Cite this

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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 journalArticle

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