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Axion model in extra dimensions with TeV scale gravity
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TU-572
Axion model in extra dimensions with TeV scale gravity
Sanghyeon Chang, Shiro Tazawa and Masahiro Yamaguchi
Department of Physics, Tohoku University, Sendai 980-8578, Japan
Abstract
A simple axion model is proposed in the scenario of large extra dimensions
where gravity scale is as low as 1 TeV. To obtain an intermediate-scale decay
constant of the axion, the axion is assumed to live in a sub-spacetime (brane)
of the whole bulk. In this model there appear Kaluza-Klein modes of the axion
which have stronger interaction than those of the graviton. The axion brane
plays a role of absorber of the graviton Kaluza-Klein modes. Because of these
reasons phenomenology and cosmology of the axion become highly non-trivial.
We discuss various cosmological constraints as well as astrophysical ones and
show that the model is viable for certain choices of the dimensionality of the
axion brane. The structure of the model proposed here provides a viable
realization of the fat brane idea to relax otherwise very severe cosmological
constraints.
Typeset using REVTEX
1
I. INTRODUCTION
It has been suggested that the fundamental scale of nature can be as low as TeV, whereas
the largeness of the effective Planck scale or the weakness of the gravity in a long distance
can be explained by introducing large extra dimensions [1–4]. When there exist n of such
extra dimensions, the relation between the gravitational constant 8πGN = 1/M
2
pl(4) in 4
dimensions and the fundamental scale Mpl(4+n) in (4 + n) dimensions is given
M2pl(4) ~ VnMn+2pl(4+n), (1)
where Vn is the volume of the extra dimensional space. For Mpl(4+n) ~ 1 TeV, the size of
the extra dimensions rn is computed as
rn ~ V 1/nn ~ 10
32
n
?6M
?
2
n
?1
TeV MeV
?1 ~ 10 32n ?17M?
2
n
?1
TeV cm, (2)
where MTeV ≡ Mpl(4+n)/TeV. The case n = 1 is excluded because the gravitational law
would change at macroscopic level, but the cases n ≥ 2 are allowed by gravity experim
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