Cosmology at high redshift — a probe of fundamental physics

An observational program focused on the high redshift (2<z<6) Universe has the opportunity to dramatically improve over upcoming LSS and CMB surveys on measurements of both the standard cosmological model and its extensions. Using a Fisher matrix formalism that builds upon recent advances in L...

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Published inJournal of cosmology and astroparticle physics Vol. 2021; no. 12; pp. 49 - 110
Main Authors Sailer, Noah, Castorina, Emanuele, Ferraro, Simone, White, Martin
Format Journal Article
LanguageEnglish
Published Bristol IOP Publishing 01.12.2021
Institute of Physics (IOP)
Subjects
Astronomical models
ASTRONOMY AND ASTROPHYSICS
Cosmic microwave background
cosmological parameters from LSS
cosmological perturbation theory
Cosmology
Cross correlation
Dark energy
Fisher information
Formalism
Galaxies
gravitational lensing
Neutrinos
Perturbation theory
Polls & surveys
Red shift
redshift surveys
Online AccessGet full text
ISSN1475-7516
1475-7516
DOI10.1088/1475-7516/2021/12/049

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Abstract An observational program focused on the high redshift (2<z<6) Universe has the opportunity to dramatically improve over upcoming LSS and CMB surveys on measurements of both the standard cosmological model and its extensions. Using a Fisher matrix formalism that builds upon recent advances in Lagrangian perturbation theory, we forecast constraints for future spectroscopic and 21-cm surveys on the standard cosmological model, curvature, neutrino mass, relativistic species, primordial features, primordial non-Gaussianity, dynamical dark energy, and gravitational slip. We compare these constraints with those achievable by current or near-future surveys such as DESI and Euclid, all under the same forecasting formalism, and compare our formalism with traditional linear methods. Our Python code FishLSS — used to calculate the Fisher information of the full shape power spectrum, CMB lensing, the cross-correlation of CMB lensing with galaxies, and combinations thereof — is publicly available.
AbstractList An observational program focused on the high redshift (2<z<6) Universe has the opportunity to dramatically improve over upcoming LSS and CMB surveys on measurements of both the standard cosmological model and its extensions. Using a Fisher matrix formalism that builds upon recent advances in Lagrangian perturbation theory, we forecast constraints for future spectroscopic and 21-cm surveys on the standard cosmological model, curvature, neutrino mass, relativistic species, primordial features, primordial non-Gaussianity, dynamical dark energy, and gravitational slip. We compare these constraints with those achievable by current or near-future surveys such as DESI and Euclid, all under the same forecasting formalism, and compare our formalism with traditional linear methods. Here, our Python code FishLSS — used to calculate the Fisher information of the full shape power spectrum, CMB lensing, the cross-correlation of CMB lensing with galaxies, and combinations thereof — is publicly available.
An observational program focused on the high redshift (2<z<6) Universe has the opportunity to dramatically improve over upcoming LSS and CMB surveys on measurements of both the standard cosmological model and its extensions. Using a Fisher matrix formalism that builds upon recent advances in Lagrangian perturbation theory, we forecast constraints for future spectroscopic and 21-cm surveys on the standard cosmological model, curvature, neutrino mass, relativistic species, primordial features, primordial non-Gaussianity, dynamical dark energy, and gravitational slip. We compare these constraints with those achievable by current or near-future surveys such as DESI and Euclid, all under the same forecasting formalism, and compare our formalism with traditional linear methods. Our Python code FishLSS — used to calculate the Fisher information of the full shape power spectrum, CMB lensing, the cross-correlation of CMB lensing with galaxies, and combinations thereof — is publicly available.
An observational program focused on the high redshift (2<z<6) Universe has the opportunity to dramatically improve over upcoming LSS and CMB surveys on measurements of both the standard cosmological model and its extensions. Using a Fisher matrix formalism that builds upon recent advances in Lagrangian perturbation theory, we forecast constraints for future spectroscopic and 21-cm surveys on the standard cosmological model, curvature, neutrino mass, relativistic species, primordial features, primordial non-Gaussianity, dynamical dark energy, and gravitational slip. We compare these constraints with those achievable by current or near-future surveys such as DESI and Euclid, all under the same forecasting formalism, and compare our formalism with traditional linear methods. Our Python code FishLSS — used to calculate the Fisher information of the full shape power spectrum, CMB lensing, the cross-correlation of CMB lensing with galaxies, and combinations thereof — is publicly available.
Author Sailer, Noah
Castorina, Emanuele
White, Martin
Ferraro, Simone
Author_xml – sequence: 1
  givenname: Noah
  surname: Sailer
  fullname: Sailer, Noah
  organization: Berkeley Center for Cosmological Physics, UC Berkeley, Berkeley, CA 94720, U.S.A
– sequence: 2
  givenname: Emanuele
  surname: Castorina
  fullname: Castorina, Emanuele
  organization: Theoretical Physics Department, CERN, 1211 Geneva 23, Switzerland
– sequence: 3
  givenname: Simone
  surname: Ferraro
  fullname: Ferraro, Simone
  organization: Lawrence Berkeley National Laboratory, One Cyclotron Road, Berkeley, CA 94720, U.S.A
– sequence: 4
  givenname: Martin
  surname: White
  fullname: White, Martin
  organization: Lawrence Berkeley National Laboratory, One Cyclotron Road, Berkeley, CA 94720, U.S.A
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Snippet An observational program focused on the high redshift (2<z<6) Universe has the opportunity to dramatically improve over upcoming LSS and CMB surveys on...
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SubjectTerms Astronomical models
ASTRONOMY AND ASTROPHYSICS
Cosmic microwave background
cosmological parameters from LSS
cosmological perturbation theory
Cosmology
Cross correlation
Dark energy
Fisher information
Formalism
Galaxies
gravitational lensing
Neutrinos
Perturbation theory
Polls & surveys
Red shift
redshift surveys
Title Cosmology at high redshift — a probe of fundamental physics
URI https://iopscience.iop.org/article/10.1088/1475-7516/2021/12/049
https://www.proquest.com/docview/2612080091
https://www.osti.gov/servlets/purl/1876396
Volume 2021
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