• Corpus ID: 17265901

Fundamental Field Theory in Ten Dimensions and The Early Universe

@article{Patwardhan2006FundamentalFT,
  title={Fundamental Field Theory in Ten Dimensions and The Early Universe},
  author={Ajay Patwardhan},
  journal={arXiv: High Energy Physics - Theory},
  year={2006}
}
  • A. Patwardhan
  • Published 9 June 2006
  • Physics
  • arXiv: High Energy Physics - Theory
A unified field theory in ten dimensions, of all interactions, can describe high energy processes occuring in the early universe. In such a theory transitions that give properties of the universe can occur due to the presence of algebraic and geometric structures. A correspondence between theory and observations of the universe is made, to obtain a new interpretation and properties. This paper consists of a field theory and cosmological model of dark and normal energy and matter, cosmological… 

References

SHOWING 1-10 OF 12 REFERENCES

Quantum Fields in Curved Space

This book presents a comprehensive review of the subject of gravitational effects in quantum field theory. Although the treatment is general, special emphasis is given to the Hawking black hole

The Cosmological Constant and Dark Energy

Physics invites the idea that space contains energy whose gravitational effect approximates that of Einstein's cosmological constant, Lambda: nowadays the concept is termed dark energy or

Supersymmetric quantum cosmology

We address the canonical quantization in the framework of N = 1 simple supergravity for the case of Gowdy T3 cosmological models. It will be proved that there exist physical states in the

The Casimir Effect and Its Applications

The Casimir effect is analyzed. This effect consists of a polarization of the vacuum of quantized fields which arises as a result of a change in the spectrum of vacuum oscillations when the

The breakdown of topology at small scales

We discuss how a topology (the Zariski topology) on a space can appear to break down at small distances due to D-brane decay. The mechanism proposed coincides perfectly with the phase picture of

Three-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Implications for Cosmology

A simple cosmological model with only six parameters (matter density, Ωmh2, baryon density, Ωbh2, Hubble constant, H0, amplitude of fluctuations, σ8, optical depth, τ, and a slope for the scalar

Task force on cosmic microwave background research

One of the most spectacular scientific breakthroughs in past decades was using measurements of the fluctuations in the cosmic microwave background (CMB) to test precisely our understanding of the

Update on the direct detection of supersymmetric dark matter

We compare updated predictions for the elastic scattering of supersymmetric neutralino dark matter with the improved experimental upper limit recently published by Cryogenic Dark Matter Search (CDMS)

Physics Reports

  • Education