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August 2011 |
The Zel'dovich approximation
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February 2014 |
An analytic model for the spatial clustering of dark matter haloes
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A perturbative approach to the redshift space correlation function: beyond the Standard Model
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August 2017 |
Efficient Computation of Cosmic Microwave Background Anisotropies in Closed Friedmann‐Robertson‐Walker Models
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August 2000 |
Biasing and the distribution of dark matter haloes
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April 1999 |
Environmental dependence of masses and coupling constants
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February 2008 |
Planck 2013 results. XVI. Cosmological parameters
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October 2014 |
The Gaussian streaming model and convolution Lagrangian effective field theory
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December 2016 |
Is cosmic speed-up due to new gravitational physics?
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August 2004 |
Critical look at cosmological perturbation theory techniques
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August 2009 |
Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes
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May 2001 |
The one-loop matter bispectrum as a probe of gravity and dark energy
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October 2018 |
Comparing halo bias from abundance and clustering
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April 2015 |
Nonlinear evolution of the matter power spectrum in modified theories of gravity
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June 2009 |
Tests of chameleon gravity
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March 2018 |
Halo model and halo properties in Galileon gravity cosmologies
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April 2014 |
A marked correlation function for constraining modified gravity models
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November 2016 |
Planck 2015 results : XIII. Cosmological parameters
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September 2016 |
Excursion set theory for modified gravity: Eulerian versus Lagrangian environments: Excursion set in modified gravity reload
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July 2012 |
On the spatial correlations of Abell clusters
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September 1984 |
Large-scale bias and the inaccuracy of the peak-background split: Large-scale bias
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December 2009 |
Dark Energy after GW170817 and GRB170817A
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December 2017 |
Models of cosmic acceleration that evade solar system tests
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September 2007 |
Implications of the Neutron Star Merger GW170817 for Cosmological Scalar-Tensor Theories
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December 2017 |
Dark Energy After GW170817: Dead Ends and the Road Ahead
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December 2017 |
Cosmological hydrodynamics with adaptive mesh refinement: A new high resolution code called RAMSES
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April 2002 |
Excursion set mass functions for hierarchical Gaussian fluctuations
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September 1991 |
Gravitational clustering from scale-free initial conditions
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December 1988 |
Type Ia Supernova Discoveries at z > 1 from the Hubble Space Telescope : Evidence for Past Deceleration and Constraints on Dark Energy Evolution
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June 2004 |
Recursive solutions of Lagrangian perturbation theory
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July 2015 |
Peak-background split, renormalization, and galaxy clustering
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July 2013 |
An Ordinary Short Gamma-Ray Burst with Extraordinary Implications: Fermi -GBM Detection of GRB 170817A
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October 2017 |
Halo models of large scale structure
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December 2002 |
Deriving the Nonlinear Cosmological Power Spectrum and Bispectrum from Analytic Dark Matter Halo Profiles and Mass Functions
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November 2000 |
Strong Constraints on Cosmological Gravity from GW170817 and GRB 170817A
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December 2017 |
Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS
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August 2009 |
The modified gravity light-cone simulation project – I. Statistics of matter and halo distributions
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November 2018 |
Exploring Vainshtein mechanism on adaptively refined meshes
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May 2013 |
Convolution Lagrangian perturbation theory for biased tracers
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December 2012 |
The Halo Occupation Distribution: Toward an Empirical Determination of the Relation between Galaxies and Mass
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August 2002 |
Impact on the power spectrum of screening in modified gravity scenarios
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July 2013 |
NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: COSMOLOGICAL PARAMETER RESULTS
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September 2013 |
Lagrangian or Eulerian; real or Fourier? Not all approaches to large-scale structure are created equal
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June 2014 |
Multi-messenger Observations of a Binary Neutron Star Merger
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October 2017 |
Testing general relativity in cosmology
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December 2018 |
Chameleon cosmology
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February 2004 |
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
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June 1999 |
The Confrontation between General Relativity and Experiment
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March 2006 |
Erratum: Nonlinear perturbation theory with halo bias and redshift-space distortions via the Lagrangian picture [Phys. Rev. D 78 , 083519 (2008)]
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November 2008 |
Nonlinear perturbation theory with halo bias and redshift-space distortions via the Lagrangian picture
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October 2008 |
From -essence to generalized Galileons
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September 2011 |
Beyond consistency test of gravity with redshift-space distortions at quasilinear scales
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February 2014 |
No-Go Theorems for Generalized Chameleon Field Theories
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December 2012 |
Chameleon Fields: Awaiting Surprises for Tests of Gravity in Space
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October 2004 |
Large-scale bias and the peak background split
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September 1999 |
Nonlinear evolution of initially biased tracers in modified gravity
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November 2018 |
Revealing modified gravity signals in matter and halo hierarchical clustering
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July 2017 |
The statistics of peaks of Gaussian random fields
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To the problem of nonvanishing gravitation mass
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Cosmological tests of modified gravity
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March 2016 |
Efficient simulations of large-scale structure in modified gravity cosmologies with comoving Lagrangian acceleration
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May 2017 |
An introduction to the Vainshtein mechanism
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September 2013 |
Speeding up N -body simulations of modified gravity: chameleon screening models
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February 2017 |
Lagrangian perturbation theory for modified gravity
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December 2017 |
The cosmological simulation code gadget-2
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December 2005 |
Large-scale galaxy bias
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February 2018 |
Screening in perturbative approaches to LSS
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October 2017 |
Measuring the Baryon Acoustic Oscillation scale using the Sloan Digital Sky Survey and 2dF Galaxy Redshift Survey: Measuring the BAO scale
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September 2007 |
4D gravity on a brane in 5D Minkowski space
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July 2000 |
The WiggleZ Dark Energy Survey: improved distance measurements to z = 1 with reconstruction of the baryonic acoustic feature
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May 2014 |
Second-order scalar-tensor field equations in a four-dimensional space
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September 1974 |
Large-scale structure of the Universe and cosmological perturbation theory
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September 2002 |
Lagrangian perturbation theory at one loop order: Successes, failures, and improvements
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January 2015 |
f(R) Theories
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June 2010 |
Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
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October 2017 |
Ghosts in the self-accelerating universe
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November 2007 |
The Santiago–Harvard–Edinburgh–Durham void comparison – I. SHEDding light on chameleon gravity tests
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February 2018 |
Non-linear cosmological power spectra in real and redshift space
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October 1996 |
High-order correlations of peaks and haloes: a step towards understanding galaxy biasing
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January 1997 |
An extended excursion set approach to structure formation in chameleon models
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January 2012 |
GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
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October 2017 |
A Lagrangian effective field theory
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September 2015 |
The Dark Side of the Halo Occupation Distribution
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July 2004 |
Excursion set theory for modified gravity: correlated steps, mass functions and halo bias: Excursion set theory for modified gravity
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October 2012 |
The cosmological constant problem
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January 1989 |
Populating a cluster of galaxies - I. Results at \fontshape{it}{z}=0
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December 2001 |
Formation of Galaxies and Clusters of Galaxies by Self-Similar Gravitational Condensation
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February 1974 |
Solving large scale structure in ten easy steps with COLA
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June 2013 |
Baryon acoustic oscillations in the Sloan Digital Sky Survey Data Release 7 galaxy sample
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February 2010 |
ECOSMOG : an Efficient COde for Simulating MOdified Gravity
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January 2012 |
A Closure Theory for Nonlinear Evolution of Cosmological Power Spectra
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February 2008 |
Halo occupation numbers and galaxy bias
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November 2000 |
The Rockstar Phase-Space Temporal halo Finder and the Velocity Offsets of Cluster Cores
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December 2012 |
How Many Galaxies Fit in a Halo? Constraints on Galaxy Formation Efficiency from Spatial Clustering
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January 2001 |
Spherical collapse in Galileon gravity: fifth force solutions, halo mass function and halo bias
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November 2013 |
gravity and chameleon theories
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November 2008 |
Theoretical Models of the Halo Occupation Distribution: Separating Central and Satellite Galaxies
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November 2005 |
Nonlinear perturbation theory integrated with nonlocal bias, redshift-space distortions, and primordial non-Gaussianity
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journal
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April 2011 |
Modified-Gravity-gadget: a new code for cosmological hydrodynamical simulations of modified gravity models
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September 2013 |
Modeling halo mass functions in chameleon gravity
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June 2013 |
UV-completion by classicalization
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August 2011 |
INTEGRAL Detection of the First Prompt Gamma-Ray Signal Coincident with the Gravitational-wave Event GW170817
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journal
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October 2017 |
Perturbation theory and excursion set estimates of the probability distribution function of dark matter, and a method for reconstructing the initial distribution function
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journal
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May 2008 |
Detection of the Baryon Acoustic Peak in the Large‐Scale Correlation Function of SDSS Luminous Red Galaxies
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November 2005 |
Regularized cosmological power spectrum and correlation function in modified gravity models
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journal
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December 2014 |
Speeding up N-body simulations of modified gravity: Vainshtein screening models
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journal
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December 2015 |
The Cosmological constant problem
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journal
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May 2004 |
Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
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text
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January 2017 |
GW170817: Observation of gravitational waves from a binary neutron star inspiral
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text
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January 2017 |
Planck 2015 results : X. Diffuse component separation: Foreground maps
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journal
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September 2016 |
The Cosmological Constant Problem
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journal
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March 2004 |
The Confrontation between General Relativity and Experiment
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journal
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June 2014 |
How to suppress the shot noise in galaxy surveys
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text
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January 2009 |
Multi-messenger Observations of a Binary Neutron Star Merger
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text
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January 2017 |
Planck 2015 results : XVI. Isotropy and statistics of the CMB
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journal
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September 2016 |
GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
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other
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January 2017 |
Planck 2015 results : XXVI. The Second
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journal
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September 2016 |
Models of f(R) Cosmic Acceleration that Evade Solar-System Tests
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text
|
January 2007 |
A Closure Theory for Non-linear Evolution of Cosmological Power Spectra
|
text
|
January 2007 |
Environmental Dependence of Masses and Coupling Constants
|
text
|
January 2007 |
Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift Space
|
text
|
January 2007 |
Perturbation theory and excursion set estimates of the probability distribution function of dark matter, and a method for reconstructing the initial distribution function
|
text
|
January 2007 |
Nonlinear perturbation theory with halo bias and redshift-space distortions via the Lagrangian picture
|
text
|
January 2008 |
A critical look at cosmological perturbation theory techniques
|
text
|
January 2009 |
Spherical Collapse and the Halo Model in Braneworld Gravity
|
text
|
January 2009 |
Nonlinear Perturbation Theory Integrated with Nonlocal Bias, Redshift-space Distortions, and Primordial Non-Gaussianity
|
text
|
January 2011 |
From k-essence to generalised Galileons
|
text
|
January 2011 |
The Rockstar Phase-Space Temporal Halo Finder and the Velocity Offsets of Cluster Cores
|
text
|
January 2011 |
No-Go Theorems for Generalized Chameleon Field Theories
|
text
|
January 2012 |
Convolution Lagrangian perturbation theory for biased tracers
|
text
|
January 2012 |
Peak-Background Split, Renormalization, and Galaxy Clustering
|
text
|
January 2012 |
Solving Large Scale Structure in Ten Easy Steps with COLA
|
text
|
January 2013 |
Planck 2013 results. XVI. Cosmological parameters
|
text
|
January 2013 |
Modified Gravity-GADGET: A new code for cosmological hydrodynamical simulations of modified gravity models
|
text
|
January 2013 |
Impact on the power spectrum of Screening in Modified Gravity Scenarios
|
text
|
January 2013 |
Spherical collapse in Galileon gravity: fifth force solutions, halo mass function and halo bias
|
text
|
January 2013 |
Lagrangian or Eulerian; Real or Fourier? Not All Approaches to Large-Scale Structure Are Created Equal
|
text
|
January 2013 |
The Zeldovich approximation
|
text
|
January 2014 |
Regularized cosmological power spectrum and correlation function in modified gravity models
|
text
|
January 2014 |
Lagrangian perturbation theory at one loop order: successes, failures, and improvements
|
text
|
January 2014 |
Planck 2015 results. XIII. Cosmological parameters
|
text
|
January 2015 |
Recursive Solutions of Lagrangian Perturbation Theory
|
text
|
January 2015 |
A Lagrangian effective field theory
|
text
|
January 2015 |
A marked correlation function for constraining modified gravity models
|
text
|
January 2016 |
Speeding up $N$-body simulations of modified gravity: Chameleon screening models
|
text
|
January 2016 |
Large-Scale Galaxy Bias
|
text
|
January 2016 |
Efficient simulations of large scale structure in modified gravity cosmologies with comoving Lagrangian acceleration
|
text
|
January 2016 |
A Perturbative Approach to the Redshift Space Correlation Function: Beyond the Standard Model
|
text
|
January 2017 |
An Ordinary Short Gamma-Ray Burst with Extraordinary Implications: Fermi-GBM Detection of GRB 170817A
|
text
|
January 2017 |
INTEGRAL Detection of the First Prompt Gamma-Ray Signal Coincident with the Gravitational Wave Event GW170817
|
text
|
January 2017 |
GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
|
text
|
January 2017 |
Dark Energy after GW170817: dead ends and the road ahead
|
text
|
January 2017 |
Strong constraints on cosmological gravity from GW170817 and GRB 170817A
|
text
|
January 2017 |
The modified gravity lightcone simulation project I: Statistics of matter and halo distributions
|
text
|
January 2018 |
The one-loop matter bispectrum as a probe of gravity and dark energy
|
text
|
January 2018 |
Nonlinear evolution of initially biased tracers in modified gravity
|
text
|
January 2018 |
Halo occupation numbers and galaxy bias
|
text
|
January 2000 |
How Many Galaxies Fit in a Halo? Constraints on Galaxy Formation Efficiency from Spatial Clustering
|
text
|
January 2000 |
Large-Scale Structure of the Universe and Cosmological Perturbation Theory
|
text
|
January 2001 |
The Dark Side of the Halo Occupation Distribution
|
text
|
January 2003 |
Chameleon Cosmology
|
text
|
January 2003 |
Theoretical Models of the Halo Occupation Distribution: Separating Central and Satellite Galaxies
|
text
|
January 2004 |
An analytic model for the spatial clustering of dark matter haloes
|
text
|
January 1995 |
High-Order Correlations of Peaks and Halos: a Step toward Understanding Galaxy Biasing
|
text
|
January 1996 |
The Confrontation between General Relativity and Experiment
|
text
|
January 2001 |