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Иш: D-brane and exponential potentials inspire warm inflation and swampland conjecture

  1. Measurements of Ω and Λ from 42 High‐Redshift Supernovae

    S. Perlmutter, G. Aldering, G. Goldhaber +30

    Мақола1999103 иқтибос
    ABI
  2. <i>Planck</i> 2018 results

    N. Aghanim, Y. Akrami, M. Ashdown +97

    Мақола202090 иқтибос
    ABI
  3. The cosmological constant problem

    Steven Weinberg

    Мақола198954 иқтибос
    ABI
  4. Generalized Chaplygin gas, accelerated expansion, and dark-energy-matter unification

    M. C. Bento, Orfeu Bertolami, Anjan A. Sen

    Мақола200230 иқтибос
    ABI
  5. Сарлавҳасиз

    Бошқа25 иқтибос
    ABI
  6. A new type of isotropic cosmological models without singularity

    Alexei A. Starobinsky

    Мақола198024 иқтибос
    ABI
  7. Сарлавҳасиз

    Бошқа19 иқтибос
    ABI
  8. THE CASE FOR A POSITIVE COSMOLOGICAL Λ-TERM

    Varun Sahni, Alexei A. Starobinsky

    Мақола200016 иқтибос
    ABI
  9. Inflationary universe: A possible solution to the horizon and flatness problems

    Alan H. Guth

    Мақола198115 иқтибос
    ABI
  10. Holographic Chaplygin gas model

    M. R. Setare

    Мақола20077 иқтибос
    ABI
  11. <i>Planck</i>2018 results

    Y. Akrami, F. Arroja, M. Ashdown +97

    Мақола20193 иқтибос
    ABI
  12. Inflationary Cosmology in Modified Gravity Theories

    Kazuharu Bamba, Sergei Odintsov

    Мақола20153 иқтибос
    ABI
  13. Swampland criteria of inflationary scalar field models with well-known potentials

    Shamaila Rani, Abdul Jawad, Abdul Malik Sultan +1

    Мақола20223 иқтибос
    ABI
  14. The expansion of the Universe is faster than expected

    Adam G. Riess

    Шарҳ мақола20192 иқтибос
    ABI
  15. Сарлавҳасиз

    Бошқа2 иқтибос
    ABI
  16. Interacting modified variable Chaplygin gas in a non-flat universe

    Mubasher Jamil, Muneer Ahmad Rashid

    Мақола20082 иқтибос
    ABI
  17. Сарлавҳасиз

    Бошқа2 иқтибос
    ABI
  18. Сарлавҳасиз

    Бошқа1 иқтибос
    ABI
  19. Сарлавҳасиз

    Бошқа1 иқтибос
    ABI