Phenomenology of Randall-Sundrum Black Holes

Luis A. Anchordoqui; Haim Goldberg; Alfred D. Shapere

doi:10.1103/PhysRevD.66.024033

Phenomenology of Randall-Sundrum Black Holes

Luis A. Anchordoqui, Haim Goldberg, Alfred D. Shapere

Physics And Astronomy

Research output: Contribution to journal › Article › peer-review

28 Scopus citations

28 Downloads (Pure)

Abstract

We explore the phenomenology of microscopic black holes in the $S^1/Z_2$ Randall-Sundrum (RS) model. We consider the canonical framework in which both gauge and matter fields are confined to the brane and only gravity spills into the extra dimension. The model is characterized by two parameters, the mass of the first massive graviton $(m_1)$, and the curvature $1/\ell$ of the RS anti-de Sitter space. We compute the sensitivity of present and future cosmic ray experiments to various regions of $\ell$ and $m_1,$ and compare with that of Runs I and II at the Tevatron. As part of our phenomenological analysis, we examine constraints placed on $\ell$ by AdS/CFT considerations.

Original language	Undefined/Unknown
Journal	Phys.Rev. D
DOIs	https://doi.org/10.1103/PhysRevD.66.024033
State	Published - Apr 19 2002

Bibliographical note

Version to appear in Physical Review D; contains additional analysis on sensitivity of OWL

Keywords

hep-ph
astro-ph
gr-qc
hep-ex
hep-th

Access to Document

10.1103/PhysRevD.66.024033

0204228v3

Cite this

@article{4517d48140784b19a608ef434f4ca3e8,

title = "Phenomenology of Randall-Sundrum Black Holes",

abstract = " We explore the phenomenology of microscopic black holes in the $S^1/Z_2$ Randall-Sundrum (RS) model. We consider the canonical framework in which both gauge and matter fields are confined to the brane and only gravity spills into the extra dimension. The model is characterized by two parameters, the mass of the first massive graviton $(m_1)$, and the curvature $1/\ell$ of the RS anti-de Sitter space. We compute the sensitivity of present and future cosmic ray experiments to various regions of $\ell$ and $m_1,$ and compare with that of Runs I and II at the Tevatron. As part of our phenomenological analysis, we examine constraints placed on $\ell$ by AdS/CFT considerations. ",

keywords = "hep-ph, astro-ph, gr-qc, hep-ex, hep-th",

author = "Anchordoqui, {Luis A.} and Haim Goldberg and Shapere, {Alfred D.}",

note = "Version to appear in Physical Review D; contains additional analysis on sensitivity of OWL",

year = "2002",

month = apr,

day = "19",

doi = "10.1103/PhysRevD.66.024033",

language = "Undefined/Unknown",

}

TY - JOUR

T1 - Phenomenology of Randall-Sundrum Black Holes

AU - Anchordoqui, Luis A.

AU - Goldberg, Haim

AU - Shapere, Alfred D.

N1 - Version to appear in Physical Review D; contains additional analysis on sensitivity of OWL

PY - 2002/4/19

Y1 - 2002/4/19

N2 - We explore the phenomenology of microscopic black holes in the $S^1/Z_2$ Randall-Sundrum (RS) model. We consider the canonical framework in which both gauge and matter fields are confined to the brane and only gravity spills into the extra dimension. The model is characterized by two parameters, the mass of the first massive graviton $(m_1)$, and the curvature $1/\ell$ of the RS anti-de Sitter space. We compute the sensitivity of present and future cosmic ray experiments to various regions of $\ell$ and $m_1,$ and compare with that of Runs I and II at the Tevatron. As part of our phenomenological analysis, we examine constraints placed on $\ell$ by AdS/CFT considerations.

AB - We explore the phenomenology of microscopic black holes in the $S^1/Z_2$ Randall-Sundrum (RS) model. We consider the canonical framework in which both gauge and matter fields are confined to the brane and only gravity spills into the extra dimension. The model is characterized by two parameters, the mass of the first massive graviton $(m_1)$, and the curvature $1/\ell$ of the RS anti-de Sitter space. We compute the sensitivity of present and future cosmic ray experiments to various regions of $\ell$ and $m_1,$ and compare with that of Runs I and II at the Tevatron. As part of our phenomenological analysis, we examine constraints placed on $\ell$ by AdS/CFT considerations.

KW - hep-ph

KW - astro-ph

KW - gr-qc

KW - hep-ex

KW - hep-th

U2 - 10.1103/PhysRevD.66.024033

DO - 10.1103/PhysRevD.66.024033

M3 - Article

JO - Phys.Rev. D

JF - Phys.Rev. D

ER -

Phenomenology of Randall-Sundrum Black Holes

Abstract

Bibliographical note

Keywords

Access to Document

Fingerprint

Cite this