### Abstract

We study some of the novel effects that arise when the QCD axion is placed in the "bulk" of large extra spacetime dimensions. First, we find that the mass of the axion can become independent of the energy scale associated with the breaking of the Peccei-Quinn symmetry. This implies that the mass of the axion can be adjusted independently of its couplings to ordinary matter, a feature which is not possible in four dimensions and which may contribute to axion invisibility. Second, we discuss the new phenomenon of laboratory axion oscillations (analogous to neutrino oscillations), and show that these oscillations cause laboratory axions to "decohere" extremely rapidly as a result of Kaluza-Klein mixing. This decoherence may also be a contributing factor to axion invisibility. Third, we discuss the role of Kaluza-Klein axions in axion-mediated processes and decays, and propose several experimental tests of the higher-dimensional nature of the axion. Finally, we show that under certain circumstances the presence of an infinite tower of Kaluza-Klein axion modes can significantly accelerate the dissipation of the energy associated with cosmological relic axion oscillations, thereby enabling the Peccei-Quinn symmetry-breaking scale to exceed the usual four-dimensional relic oscillation bounds. Together, these ideas therefore provide new ways of obtaining an "invisible" axion within the context of higher-dimensional theories with large-radius compactifications.

Original language | English (US) |
---|---|

Article number | 105023 |

Pages (from-to) | 1-22 |

Number of pages | 22 |

Journal | Physical Review D - Particles, Fields, Gravitation and Cosmology |

Volume | 62 |

Issue number | 10 |

State | Published - Nov 15 2000 |

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### ASJC Scopus subject areas

- Physics and Astronomy(all)
- Nuclear and High Energy Physics
- Mathematical Physics
- Physics and Astronomy (miscellaneous)

### Cite this

*Physical Review D - Particles, Fields, Gravitation and Cosmology*,

*62*(10), 1-22. [105023].

**Invisible axions and large-radius compactifications.** / Dienes, Keith R; Dudas, Emilian; Gherghetta, Tony.

Research output: Contribution to journal › Article

*Physical Review D - Particles, Fields, Gravitation and Cosmology*, vol. 62, no. 10, 105023, pp. 1-22.

}

TY - JOUR

T1 - Invisible axions and large-radius compactifications

AU - Dienes, Keith R

AU - Dudas, Emilian

AU - Gherghetta, Tony

PY - 2000/11/15

Y1 - 2000/11/15

N2 - We study some of the novel effects that arise when the QCD axion is placed in the "bulk" of large extra spacetime dimensions. First, we find that the mass of the axion can become independent of the energy scale associated with the breaking of the Peccei-Quinn symmetry. This implies that the mass of the axion can be adjusted independently of its couplings to ordinary matter, a feature which is not possible in four dimensions and which may contribute to axion invisibility. Second, we discuss the new phenomenon of laboratory axion oscillations (analogous to neutrino oscillations), and show that these oscillations cause laboratory axions to "decohere" extremely rapidly as a result of Kaluza-Klein mixing. This decoherence may also be a contributing factor to axion invisibility. Third, we discuss the role of Kaluza-Klein axions in axion-mediated processes and decays, and propose several experimental tests of the higher-dimensional nature of the axion. Finally, we show that under certain circumstances the presence of an infinite tower of Kaluza-Klein axion modes can significantly accelerate the dissipation of the energy associated with cosmological relic axion oscillations, thereby enabling the Peccei-Quinn symmetry-breaking scale to exceed the usual four-dimensional relic oscillation bounds. Together, these ideas therefore provide new ways of obtaining an "invisible" axion within the context of higher-dimensional theories with large-radius compactifications.

AB - We study some of the novel effects that arise when the QCD axion is placed in the "bulk" of large extra spacetime dimensions. First, we find that the mass of the axion can become independent of the energy scale associated with the breaking of the Peccei-Quinn symmetry. This implies that the mass of the axion can be adjusted independently of its couplings to ordinary matter, a feature which is not possible in four dimensions and which may contribute to axion invisibility. Second, we discuss the new phenomenon of laboratory axion oscillations (analogous to neutrino oscillations), and show that these oscillations cause laboratory axions to "decohere" extremely rapidly as a result of Kaluza-Klein mixing. This decoherence may also be a contributing factor to axion invisibility. Third, we discuss the role of Kaluza-Klein axions in axion-mediated processes and decays, and propose several experimental tests of the higher-dimensional nature of the axion. Finally, we show that under certain circumstances the presence of an infinite tower of Kaluza-Klein axion modes can significantly accelerate the dissipation of the energy associated with cosmological relic axion oscillations, thereby enabling the Peccei-Quinn symmetry-breaking scale to exceed the usual four-dimensional relic oscillation bounds. Together, these ideas therefore provide new ways of obtaining an "invisible" axion within the context of higher-dimensional theories with large-radius compactifications.

UR - http://www.scopus.com/inward/record.url?scp=17044420910&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=17044420910&partnerID=8YFLogxK

M3 - Article

AN - SCOPUS:17044420910

VL - 62

SP - 1

EP - 22

JO - Physical review D: Particles and fields

JF - Physical review D: Particles and fields

SN - 0556-2821

IS - 10

M1 - 105023

ER -