Brane interaction as the origin of inflation

By N. Jones, Horace Stoica, S. Tye. 2002

269 citations recorded by the source corpus.

We reanalyze brane inflation with brane-brane interactions at an angle, which include the special case of brane-anti-brane interaction. If nature is described by a stringy realization of the brane world scenario today (with arbitrary compactification), and if some additional branes were present in the early universe, we find that an inflationary epoch is generically quite natural, ending with a big bang when the last branes collide. In an interesting brane inflationary scenario suggested by generic string model-building, we use the density perturbation observed in the cosmic microwave background and the coupling unification to find that the string scale is comparable to the GUT scale.

Subfields: Astronomy and Astrophysics, Instrumentation, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/a1eb6f19e52e84df03e7c32bcd436a8480283563

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In Astronomy and Astrophysics

  1. Andrei Linde
  2. R. Kallosh
  3. Liam McAllister
  4. F. Quevedo
  5. E. Silverstein
  6. D. Baumann
  7. S. Kachru
  8. J. Polchinski

In Instrumentation

  1. F. Quevedo
  2. Andrei Linde
  3. Lev Kofman
  4. Liam McAllister
  5. S. Kachru

In Nuclear and High Energy Physics

  1. Andrei Linde
  2. R. Kallosh
  3. Liam McAllister
  4. F. Quevedo
  5. E. Silverstein
  6. D. Baumann
  7. S. Kachru
  8. Eran Palti

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