N-body light-cone mocks show 2-4 sigma deviations in third-order angular clustering between LCDM and f(R)/nDGP models at z=0.15-0.3 for halos and galaxies, with stronger signals in the dark-matter field.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
citation-role summary
background 1
citation-polarity summary
verdicts
UNVERDICTED 2roles
background 1polarities
background 1representative citing papers
F(R)-phantom BTZ black holes satisfy the first law, undergo second-order phase transitions confirmed by Ehrenfest relations, and support stable circular orbits for massive and massless particles only in the phantom regime with negative curvature.
citing papers explorer
-
Galaxy and halo angular clustering in LCDM and Modified Gravity cosmologies
N-body light-cone mocks show 2-4 sigma deviations in third-order angular clustering between LCDM and f(R)/nDGP models at z=0.15-0.3 for halos and galaxies, with stronger signals in the dark-matter field.
-
Thermodynamics, Phase Transitions, and Geodesic Structure of $F(R)-$Phantom BTZ Black Holes
F(R)-phantom BTZ black holes satisfy the first law, undergo second-order phase transitions confirmed by Ehrenfest relations, and support stable circular orbits for massive and massless particles only in the phantom regime with negative curvature.