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Curvaton (English Wikipedia)

Analysis of information sources in references of the Wikipedia article "Curvaton" in English language version.

refsWebsite
Global rank English rank
3arxiv.org
69th place
59th place
3harvard.edu
18th place
17th place
3doi.org
2nd place
2nd place
3semanticscholar.org
11th place
8th place

arxiv.org

  • Enqvist & Sloth (2002). "Adiabatic CMB perturbations in pre-Big Bang string cosmology". Nuclear Physics B. 626 (1–2): 395–409. arXiv:hep-ph/0109214. Bibcode:2002NuPhB.626..395E. doi:10.1016/S0550-3213(02)00043-3. S2CID 9320517.
  • Lyth & Wands (2002). "Generating the curvature perturbation without an inflaton". Physics Letters B. 524 (1–2): 5–14. arXiv:hep-ph/0110002. Bibcode:2002PhLB..524....5L. doi:10.1016/S0370-2693(01)01366-1. S2CID 119499489.
  • Moroi & Takahashi (2001). "Effects of Cosmological Moduli Fields on Cosmic Microwave Background". Physics Letters B. 522 (3–4): 215–221. arXiv:hep-ph/0110096. Bibcode:2001PhLB..522..215M. doi:10.1016/S0370-2693(01)01295-3. S2CID 6685102.

doi.org

  • Enqvist & Sloth (2002). "Adiabatic CMB perturbations in pre-Big Bang string cosmology". Nuclear Physics B. 626 (1–2): 395–409. arXiv:hep-ph/0109214. Bibcode:2002NuPhB.626..395E. doi:10.1016/S0550-3213(02)00043-3. S2CID 9320517.
  • Lyth & Wands (2002). "Generating the curvature perturbation without an inflaton". Physics Letters B. 524 (1–2): 5–14. arXiv:hep-ph/0110002. Bibcode:2002PhLB..524....5L. doi:10.1016/S0370-2693(01)01366-1. S2CID 119499489.
  • Moroi & Takahashi (2001). "Effects of Cosmological Moduli Fields on Cosmic Microwave Background". Physics Letters B. 522 (3–4): 215–221. arXiv:hep-ph/0110096. Bibcode:2001PhLB..522..215M. doi:10.1016/S0370-2693(01)01295-3. S2CID 6685102.

harvard.edu

ui.adsabs.harvard.edu

  • Enqvist & Sloth (2002). "Adiabatic CMB perturbations in pre-Big Bang string cosmology". Nuclear Physics B. 626 (1–2): 395–409. arXiv:hep-ph/0109214. Bibcode:2002NuPhB.626..395E. doi:10.1016/S0550-3213(02)00043-3. S2CID 9320517.
  • Lyth & Wands (2002). "Generating the curvature perturbation without an inflaton". Physics Letters B. 524 (1–2): 5–14. arXiv:hep-ph/0110002. Bibcode:2002PhLB..524....5L. doi:10.1016/S0370-2693(01)01366-1. S2CID 119499489.
  • Moroi & Takahashi (2001). "Effects of Cosmological Moduli Fields on Cosmic Microwave Background". Physics Letters B. 522 (3–4): 215–221. arXiv:hep-ph/0110096. Bibcode:2001PhLB..522..215M. doi:10.1016/S0370-2693(01)01295-3. S2CID 6685102.

semanticscholar.org

api.semanticscholar.org

  • Enqvist & Sloth (2002). "Adiabatic CMB perturbations in pre-Big Bang string cosmology". Nuclear Physics B. 626 (1–2): 395–409. arXiv:hep-ph/0109214. Bibcode:2002NuPhB.626..395E. doi:10.1016/S0550-3213(02)00043-3. S2CID 9320517.
  • Lyth & Wands (2002). "Generating the curvature perturbation without an inflaton". Physics Letters B. 524 (1–2): 5–14. arXiv:hep-ph/0110002. Bibcode:2002PhLB..524....5L. doi:10.1016/S0370-2693(01)01366-1. S2CID 119499489.
  • Moroi & Takahashi (2001). "Effects of Cosmological Moduli Fields on Cosmic Microwave Background". Physics Letters B. 522 (3–4): 215–221. arXiv:hep-ph/0110096. Bibcode:2001PhLB..522..215M. doi:10.1016/S0370-2693(01)01295-3. S2CID 6685102.