scholarly journals Revealing the nonadiabatic nature of dark energy perturbations from galaxy clustering data

2017 ◽  
Vol 96 (8) ◽  
Author(s):  
Hermano Velten ◽  
Raquel Fazolo
Keyword(s):  
Dark Energy ◽  
Galaxy Clustering ◽  
Clustering Data

scholarly journals Dark Energy Survey year 1 results: Joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions

2019 ◽  
Vol 100 (2) ◽  
Author(s):  
T. M. C. Abbott ◽  
F. B. Abdalla ◽  
A. Alarcon ◽  
S. Allam ◽  
J. Annis ◽  
...  
Keyword(s):  
Dark Energy ◽  
Joint Analysis ◽  
Galaxy Clustering ◽  
Dark Energy Survey ◽  
Energy Survey

scholarly journals Joint analysis of galaxy-galaxy lensing and galaxy clustering: Methodology and forecasts for Dark Energy Survey

2016 ◽  
Vol 94 (6) ◽  
Author(s):  
Y. Park ◽  
E. Krause ◽  
S. Dodelson ◽  
B. Jain ◽  
A. Amara ◽  
...  
Keyword(s):  
Dark Energy ◽  
Joint Analysis ◽  
Galaxy Clustering ◽  
Dark Energy Survey ◽  
Energy Survey

scholarly journals Constraints on neutrino masses from Planck and Galaxy clustering data

2013 ◽  
Vol 88 (6) ◽  
Author(s):  
Elena Giusarma ◽  
Roland de Putter ◽  
Shirley Ho ◽  
Olga Mena
Keyword(s):  
Neutrino Masses ◽  
Galaxy Clustering ◽  
Clustering Data

scholarly journals Interacting dark energy from redshift-space galaxy clustering

2021 ◽  
Vol 2021 (10) ◽  
pp. 004
Author(s):  
Pedro Carrilho ◽  
Chiara Moretti ◽  
Benjamin Bose ◽  
Katarina Markovič ◽  
Alkistis Pourtsidou
Keyword(s):  
Dark Energy ◽  
Galaxy Clustering ◽  
Interacting Dark Energy

scholarly journals CONSTRAINTS ON OSCILLATING QUINTOM FROM SUPERNOVA, MICROWAVE BACKGROUND AND GALAXY CLUSTERING

2005 ◽  
Vol 20 (31) ◽  
pp. 2409-2416 ◽  
Author(s):  
JUN-QING XIA ◽  
BO FENG ◽  
XINMIN ZHANG
Keyword(s):  
Dark Energy ◽  
Equation Of State ◽  
Observational Data ◽  
Microwave Background ◽  
Galaxy Clustering ◽  
Free Parameters

We consider in this paper a simple oscillating Quintom model of dark energy which has two free parameters and an equation of state oscillating and crossing -1. For low redshifts the equation of state of this model resembles itself similar to the linearly parametrized dark energy, however differs substantially at large redshifts. We fit our model to the observational data separately from the new high redshifts supernova observations from the HST/GOODS program and previous supernova, CMB and galaxy clustering. Our results show that because of the oscillating feature of our model the constraints from observations at large redshifts such as CMB become less stringent.

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