TY - JOUR
T1 - Cargèse Lectures on Brane Induced Gravity
AU - Gabadadze, Gregory
N1 - Funding Information:
I would like to thank the organizers of the Cargèse 2007 School, especially Laurent Baulieu, Pierre Vanhove, Paul Windey, and Elena Gi-anolio. The work is supported by NASA grant NNGG05GH34G and NSF grant 0403005.
PY - 2007/9
Y1 - 2007/9
N2 - A brief introduction is given to the subject of brane induced gravity. The 5D example is discussed in detail. The 4D laws of gravity are obtained on a brane embedded in an infinite volume extra space, where the problem of stabilization of the volume modulus is absent. The theory has two classically disjoint branches of solutions - the conventional and self-accelerated one. The conventional branch is perturbatively stable, and gives rise to predictions that are potentially measurable within the Solar system. The self-accelerated branch, on the other hand, provides an existence proof for an idea that the accelerated expansion of the Universe could be due to modified gravity. This branch, however, exhibits negative mass states, suggesting that the self-accelerated solution may not be free of instabilities. A proposal to overcome this difficulty in an extension of the original model, that also allows for the quantum gravity scale to be unrestricted, is discussed.
AB - A brief introduction is given to the subject of brane induced gravity. The 5D example is discussed in detail. The 4D laws of gravity are obtained on a brane embedded in an infinite volume extra space, where the problem of stabilization of the volume modulus is absent. The theory has two classically disjoint branches of solutions - the conventional and self-accelerated one. The conventional branch is perturbatively stable, and gives rise to predictions that are potentially measurable within the Solar system. The self-accelerated branch, on the other hand, provides an existence proof for an idea that the accelerated expansion of the Universe could be due to modified gravity. This branch, however, exhibits negative mass states, suggesting that the self-accelerated solution may not be free of instabilities. A proposal to overcome this difficulty in an extension of the original model, that also allows for the quantum gravity scale to be unrestricted, is discussed.
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U2 - 10.1016/j.nuclphysbps.2007.06.005
DO - 10.1016/j.nuclphysbps.2007.06.005
M3 - Article
AN - SCOPUS:34547662768
SN - 0920-5632
VL - 171
SP - 88
EP - 98
JO - Nuclear Physics B - Proceedings Supplements
JF - Nuclear Physics B - Proceedings Supplements
IS - SPEC. ISS.
ER -