An extended excursion set approach to structure formation in chameleon models

Planckearly results. XIX. All-sky temperature and dust optical depth fromPlanckand IRAS. Constraints on the “dark gas” in our Galaxy

(2011) et al.   ASTRONOMY & ASTROPHYSICS

SEVEN-YEARWILKINSON MICROWAVE ANISOTROPY PROBE(WMAP) OBSERVATIONS: COSMOLOGICAL INTERPRETATION

(2011) E. Komatsu et al.   ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES

Scale-dependent halo bias from scale-dependent growth

(2011) Kyle Parfrey et al.   PHYSICAL REVIEW D

N-body simulations for coupled scalar-field cosmology

(2011) Baojiu Li et al.   PHYSICAL REVIEW D

N-body simulations forf(R)gravity using a self-adaptive particle-mesh code

(2011) Gong-Bo Zhao et al.   PHYSICAL REVIEW D

Nonlinear structure formation with the environmentally dependent dilaton

(2011) Philippe Brax et al.   PHYSICAL REVIEW D

The 10 Meter South Pole Telescope

(2011) J. E. Carlstrom et al.   PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC

Voids in coupled scalar field cosmology

(2010) Baojiu Li   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

Structure formation by the fifth force: Segregation of baryons and dark matter

(2010) Baojiu Li et al.   PHYSICAL REVIEW D

Dilaton and modified gravity

(2010) Philippe Brax et al.   PHYSICAL REVIEW D

Screening Long-Range Forces through Local Symmetry Restoration

(2010) Kurt Hinterbichler et al.   PHYSICAL REVIEW LETTERS

Mass functions and bias of dark matter halos

(2009) P. Valageas   ASTRONOMY & ASTROPHYSICS

Structure formation by a fifth force:N-body versus linear simulations

(2009) Baojiu Li et al.   PHYSICAL REVIEW D

Nonlinear evolution off(R)cosmologies. III. Halo statistics

(2009) Fabian Schmidt et al.   PHYSICAL REVIEW D

Spherical collapse and cluster counts in modified gravity models

(2009) Matthew C. Martino et al.   PHYSICAL REVIEW D

Nonlinear evolution off(R)cosmologies. I. Methodology

(2008) Hiroaki Oyaizu   PHYSICAL REVIEW D

Nonlinear evolution off(R)cosmologies. II. Power spectrum

(2008) Hiroaki Oyaizu et al.   PHYSICAL REVIEW D