Geometry Of Inflation

Geometry of Inflation is a theoretical framework in cosmology that specifies the spatial curvature dynamics and metric evolution during the inflationary epoch, distinguishing itself by modeling the universe's rapid exponential expansion as a geometric phase transition within general relativity.

98

Publications

4.1K

Citations

178

Authors

150

Institutions

Publications per year

2017–2026

33

Authors

178

  1. SH
    Stephen H. Shenker

    Stanford University, United States

    3 publications · 127 citations

    3

    h-index

  2. AH
    Arthur Hebecker

    Heidelberg University, Germany

    3 publications · 281 citations

    3

    h-index

  3. LS
    Leonard Susskind

    Stanford University, United States

    3 publications · 127 citations

    3

    h-index

  4. DR
    Diederik Roest

    University of Groningen, Netherlands

    3 publications · 250 citations

    3

    h-index

  5. GK
    Georgios K. Karananas

    École Polytechnique Fédérale de Lausanne, Switzerland

    1 publications · 72 citations

    2

    h-index

1–5 of 178

Venues

  1. Journal of Cosmology and Astroparticle Physics

    JCAP · 10 publications · 492 citations

    11

    h-index

  2. 11

    h-index

  3. Journal of High Energy Physics

    JHEP · 10 publications · 465 citations

    10

    h-index

  4. Physics Letters B

    9 publications · 742 citations

    10

    h-index

  5. 6

    h-index

1–5