Quantum and thermal effects in higher dimensions
Two examples of higher dimensional theories are considered at the one-loop level for quantum and thermal effects: the five dimensional Kaluza-Klein model and the 26-dimensional closed bosonic string. In the Kaluza-Klein universe with single compact spatial dimension of length L{sub 5}, the effective potential for L{sub 5} is found. If initially L{sub 5} is less than a temperature-dependent critical length, L{sub 5} will shrink at least down to a length comparable to the Planck length. This instability has been noted by Appelquist and Chodos in the zero-temperature limit. If, on the other hand, L{sub 5} starts out larger than the critical length, it will tend to increase. This result suggests that the temperature effects may play an important role in Kaluza-Klein cosmological models. The effects of quantized fermion and boson fields are then introduced. It is shown that massive fermions, as well as massive twisted bosons, can stabilize the compact fifth dimension against collapse caused by Casimir forces, provided that the sum of an induced cosmological constant and the bare cosmological constant is adjusted to be non-negative. Finally, the finite temperature string path integral for interacting closed bosonic strings is examined, following the work of Polchinski. The winding number contribution to the classical action is found for arbitrary genus. It is shown that on an arbitrary genus world sheet all windings of the fields around the compact time direction can be rotated into a single cycle. The modular invariance of this result is demonstrated.
- Research Organization:
- Texas Univ., Austin, TX (USA)
- OSTI ID:
- 5121310
- Resource Relation:
- Other Information: Thesis (Ph. D.)
- Country of Publication:
- United States
- Language:
- English
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KALUZA-KLEIN THEORY
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COSMOLOGICAL CONSTANT
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