Titlebook: Unified Symmetry; In the Small and in Behram N. Kursunoglu,Stephen Mintz,Arnold Perlmutt Book 1995 Springer Science+Business Media New Yor

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Z’ Diagnostics at Future Colliders of gauge couplings of . to quarks and leptons at the . (CERN LHC) and e.e. (NLC) colliders. For M. ~1 TeV, the NLC would have a capability to probe . the quark and lepton charges to around 10-20%, provided heavy flavor tagging and longitudinal polarization of the electron beam is available. On the

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Results from Quantum Cosmological Gravityhe Lagrangian of QCG is:. where . is Newton’s constant, A is the cosmological constant, and we employ an infinite series of local counterterms to absorb ultraviolet divergences. The astute reader will note that our metric has spacelike signature and our Riemann tensor is .

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Power Spectrum of Cosmic String Perturbations on the Microwave Background COBE data and string simulations, I derive the predicted values of (.). for several ongoing CMB experiments on medium and small angular scales. A comparison is also made with current observations and predictions of models based on inflation.

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Baryogenesis from Electroweak Strings 10. more matter than antimatter in the universe. The goal of baryogenesis is to explain why there is this asymmetry between the amount of matter and antimatter i.e. there is a nonbanishing ratio between the net baryon number density and entropy density . in the universe.

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Reconstructing the Inflaton Potentialnsity . > 0 that is positive, and results in an effective equation of state., which satisfies ä > 0. If one identifies the potential energy as arising from the potential of some scalar field ø, then ø is known as the . field.

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