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Large-scale structure formation with massive neutrinos and dynamical dark energy

Published:2014-05-13 Issue:10 Volume:89 Page:
ISSN:1550-7998
Container-title:Physical Review D
language:en
Short-container-title:Phys. Rev. D

Author:

Upadhye Amol,Biswas Rahul,Pope Adrian,Heitmann Katrin,Habib Salman,Finkel Hal,Frontiere Nicholas

Funder

U.S. Department of Energy

Publisher

American Physical Society (APS)

Subject

Nuclear and High Energy Physics

Link

http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevD.89.103515/fulltext

Reference64 articles.

1. Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant

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

3. CHANDRACLUSTER COSMOLOGY PROJECT III: COSMOLOGICAL PARAMETER CONSTRAINTS

4. SUPERNOVA CONSTRAINTS AND SYSTEMATIC UNCERTAINTIES FROM THE FIRST THREE YEARS OF THE SUPERNOVA LEGACY SURVEY

5. THEHUBBLE SPACE TELESCOPECLUSTER SUPERNOVA SURVEY. V. IMPROVING THE DARK-ENERGY CONSTRAINTS ABOVEz> 1 AND BUILDING AN EARLY-TYPE-HOSTED SUPERNOVA SAMPLE

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3. Non-linear CMB lensing with neutrinos and baryons: FLAMINGO simulations versus fast approximations;Monthly Notices of the Royal Astronomical Society;2024-03-06

4. Galaxy Clustering in the Mira-Titan Universe. I. Emulators for the Redshift Space Galaxy Correlation Function and Galaxy–Galaxy Lensing;The Astrophysical Journal;2023-07-01

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