Recombination Epoch

The Recombination Epoch is the cosmological phase in the early universe when the temperature dropped sufficiently for free electrons and protons to combine into neutral hydrogen atoms, marking the transition from an ionized plasma to a neutral intergalactic medium and enabling the decoupling of matter and radiation.

126

Publications

12.2K

Citations

373

Authors

166

Institutions

Publications per year

2017–2026

22

Variants

Recombination Era

Authors

373

  1. JC
    Jens Chluba

    University of Manchester, United Kingdom

    16 publications · 956 citations

    16

    h-index

  2. RA
    R. A. Sunyaev

    Space Research Institute, Russia

    7 publications · 450 citations

    7

    h-index

  3. SM
    S. Matarrese

    University of Padua, Italy

    4 publications · 247 citations

    4

    h-index

  4. JA
    J. A. Rubiño-Martín

    Instituto de Astrofísica de Canarias, Spain

    4 publications · 337 citations

    4

    h-index

  5. AR
    Antonio Riotto

    Istituto Nazionale di Fisica Nucleare, Sezione di Padova, Italy

    3 publications · 189 citations

    3

    h-index

1–5 of 373

Venues

  1. Monthly Notices of the Royal Astronomical Society

    23 publications · 1.2K citations

    19

    h-index

  2. The Astrophysical Journal

    ApJ · 16 publications · 6.2K citations

    14

    h-index

  3. 11

    h-index

  4. Physical review. D/Physical review. D.

    PRD · 10 publications · 803 citations

    10

    h-index

  5. Journal of Cosmology and Astroparticle Physics

    JCAP · 11 publications · 458 citations

    10

    h-index

1–5