NEUTRINO IN COSMOLOGY

By Julien Lesgourgues. 2010

208 citations recorded by the source corpus.

Subfields: Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/2e94e8efaee8dffa83f7316201bcedfb9f851389

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Nuclear and High Energy Physics

1. Julien Lesgourgues
2. S. Pastor
3. N. Palanque-Delabrouille
4. C. Yéche
5. M. Viel
6. A. Marrone
7. E. Lisi
8. V. Poulin

Citations in the corpus

• Status of Neutrino Properties and Future Prospects—Cosmological and Astrophysical Constraints (2017, background): “, [10, 12, 13] for excellent reviews on this topic).”
• On Effective Degrees of Freedom in the Early Universe (2016, background): “Other important books on the subject are written by Weinberg [6,7], Kolb and Turner [8], Dodelson [9], Ryden [10], and Lesgourgues, Mangano, Miele, and Pastor [11].”
• DEMNUni: the clustering of large-scale structures in the presence of massive neutrinos (2015, background): “Massive neutrino cosmologies have been extensively studied in the literature (see [4, 5] for a review).”
• Cosmology with massive neutrinos II: on the universality of the halo mass function and bias (2013, background): “For excellent reviews of neutrinos in cosmology see [28, 29].”
• Neutrino Mass from Cosmology (2012, methodology): “These relic processes are more efficient for larger neutrino energies, leading to non-thermal distortions in the neutrino spectra at the percent level and a slightly smaller increase of the comoving photon temperature, as noted in a series of works listed in [1, 2].”
• Neutrinoless Double Beta Decay: 2015 Review (2016, background): “A comprehensive review on the topic can be found in [137].”
• Current unknowns in the three-neutrino framework (2018, background): “Recent books with useful references on various aspects of our current understanding (and future prospects) of the neutrino mass-mixing phenomenology and its relation with astroparticle physics and cosmology include [67, 68, 69, 70, 71, 72, 73, 74, 75, 76, 77].”
• Constraint on neutrino masses from SDSS-III/BOSS Lyα forest and other cosmological probes (2014, background): “At the level of linear perturbation theory, this behavior causes a steplike suppression in the matter power spectrum, with a redshift-dependent amplitude [6, 8, 12].”
• Interacting dark sector and precision cosmology (2017, background): “Models with larger ∆N should have a smaller ratio ωb/ωcdm and a thus higher MPS amplitude on small wavelengths/large wavenumbers [41], as well as a higher CMB lensing spectrum amplitude on small angles/large multipoles.”
• Relic neutrino decoupling with flavour oscillations revisited (2016, background): “In such a case, entropy conservation leads to the well-known ratio of temperatures of relic photons and neutrinos, Tγ/Tν = (11/4) 1/3, and to a contribution of neutrinos to the cosmological energy density of radiation given, in terms of the effective number of neutrinos, by Neff = 3 [1].”
• Cosmological constraints from cosmic shear two-point correlation functions with HSC survey first-year data (2019, methodology): “For the sum of neutrino mass, we take ∑ mν = 0.06 eV from the lower bound indicated by the neutrino oscillation experiments (e.g., Lesgourgues et al. 2013, for a review) for our fiducial choice.”
• Neutrino masses and cosmology with Lyman-alpha forest power spectrum (2015, background): “power spectrum through the integrated Sachs-Wolf effect and through lensing [3, 4].”
• gevolution: a cosmological N-body code based on General Relativity (2016, background): “The consistent treatment of neutrinos within N-body simulations constitutes a difficult problem which is the domain of an entire field of research, see [51] for an overview.”
• A fresh look at linear cosmological constraints on a decaying Dark Matter component (2016, background): “Indeed, the amplitude of the matter power spectrum P (k) (expressed in units of h−3Mpc3 versus k in hMpc−1) on scales k keq depends on the primordial spectrum multiplied by (g(a0,Ωm)/Ωm)(2) [29].”
• Status of light sterile neutrino searches (2019, background): “All these quantities can be affected by the properties of relic active and sterile neutrinos [80].”