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19952026
most citedWMAP constraints on low redshift evolution of dark energy

399 citations · 1.6k across the 65 of their papers we have counts for

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25 papers · 1 filter

astro-ph2008★ 17 cited

The Adaptive TreePM: An Adaptive Resolution Code for Cosmological N-body Simulations

J. S. Bagla, Nishikanta Khandai

Cosmological N-Body simulations are used for a variety of applications. Indeed progress in the study of large scale structures and galaxy formation would have been very limited wit…

astro-ph2008★ 19 cited

Effects of the size of cosmological N-Body simulations on physical quantities - III: Skewness

J. S. Bagla, Jayanti Prasad, Nishikanta Khandai

N-Body simulations are an important tool in the study of formation of large scale structures. Much of the progress in understanding the physics of galaxy clustering and comparison…

astro-ph2008★ 10 cited

A Modified TreePM Code

Nishikanta Khandai, J. S. Bagla

We discuss the performance characteristics of using the modification of the tree code suggested by Barnes \citep{1990JCoPh..87..161B} in the context of the TreePM code. The optimis…

astro-ph2008★ 10 cited

Gravitational collapse in an expanding background and the role of substructure II: Excess power at small scales and its effect of collapse of structures at larger scales

J. S. Bagla, Jayanti Prasad

We study the interplay of clumping at small scales with the collapse and relaxation of perturbations at larger scales using N-Body simulations. We quantify the effect of collapsed…

astro-ph2007★ 40 cited

Fractal Dimensions of a Weakly Clustered Distribution and the Scale of Homogeneity

J. S. Bagla, Jaswant Yadav, T. R. Seshadri

Homogeneity and isotropy of the universe at sufficiently large scales is a fundamental premise on which modern cosmology is based. Fractal dimensions of matter distribution is a pa…

astro-ph2006★ 1 cited

Gravitational Clustering in Redshift Space: Non-Gaussian Tail of the Cosmological Density Distribution Function

J. S. Bagla, Suryadeep Ray

We study the non-Gaussian tail of the probability distribution function of density in cosmological N-Body simulations for a variety of initial conditions. We compare the behaviour…

astro-ph2006★ 25 cited

Understanding the origin of CMB constraints on Dark Energy

H. K. Jassal, J. S. Bagla, T. Padmanabhan

We study the observational constraints of CMB temperature and polarization anisotropies on models of dark energy, with special focus on models with variation in properties of dark…

astro-ph2006★ 43 cited

Effects of the size of cosmological N-Body simulations on physical quantities -- I: Mass Function

J. S. Bagla, Jayanti Prasad

N-Body simulations are a very important tool in the study of formation of large scale structures. Much of the progress in understanding the physics of galaxy formation and comparis…

astro-ph2004★ 23 cited

Cosmological N-Body Simulations

J. S. Bagla, T. Padmanabhan

In this review we discuss Cosmological N-Body codes with a special emphasis on Particle Mesh codes. We present the mathematical model for each component of N-Body codes. We compare…

astro-ph2004★ 31 cited

Cosmological N-Body simulation: Techniques, Scope and Status

J. S. Bagla

Cosmological N-Body simulations have become an essential tool for studying formation of large scale structure. These simulations are computationally challenging even though the ava…

astro-ph2004★ 45 cited

Comments on the size of the simulation box in cosmological N-Body simulations

J. S. Bagla, Suryadeep Ray

N-Body simulations are a very important tool in the study of formation of large scale structures. Much of the progress in understanding the physics of high redshift universe and co…

astro-ph2004★ 5 cited

Gravitational Collapse in an Expanding Universe: Scaling Relations for Two-Dimensional Collapse Revisited

S. Ray, J. S. Bagla, T. Padmanabhan

We investigate non-linear scaling relations for two-dimensional gravitational collapse in an expanding background using a 2D TreePM code and study the strongly non-linear regime ($…

astro-ph2004★ 8 cited

Gravitational collapse in an expanding background and the role of substructure I: Planar collapse

J. S. Bagla, Jayanti Prasad, Suryadeep Ray

We study the interplay of clumping at small scales with the collapse and relaxation of perturbations at much larger scales. We present results of our analysis when the large scale…

astro-ph2004★ 3 cited

A Parallel TreePM Code

Suryadeep Ray, J. S. Bagla

We present an algorithm for parallelising the TreePM code. We use both functional and domain decompositions. Functional decomposition is used to separate the computation of long ra…

astro-ph2004★ 399 cited

WMAP constraints on low redshift evolution of dark energy

H. K. Jassal, J. S. Bagla, T. Padmanabhan

The conceptual difficulties associated with a cosmological constant have led to the investigation of alternative models in which the equation of state parameter, , of the da…

astro-ph2002

Prospects for detecting neutral hydrogen using 21cm radiation from large scale structure at high redshifts

J. S. Bagla, Martin White

We estimate the signal from large scale structure at high redshifts in redshifted 21cm line. We focus on z ~ 3 and the LCDM cosmology. We assume that neutral hydrogen is to be foun…

astro-ph2002★ 39 cited

Performance Characteristics of TreePM codes

J. S. Bagla, Suryadeep Ray

We present a detailed analysis of the error budget for the TreePM method for doing cosmological N-Body simulations. It is shown that the choice of filter for splitting the inverse…

astro-ph2000★ 27 cited

A Comparison of Simulated and Analytic Major Merger Counts

J. D. Cohn, J. S. Bagla, Martin White

We use large volume, high resolution, N-body simulations of 3 different CDM models, with different clustering strengths, to generate dark matter halo merging histories. Over the…

astro-ph1999★ 104 cited

TreePM: A code for Cosmological N-Body Simulations

J. S. Bagla

We describe the TreePM method for carrying out large N-Body simulations to study formation and evolution of the large scale structure in the Universe. This method is a combination…

astro-ph1999★ 47 cited

The Observed Evolution of Galaxy Clustering Vs. Epoch-Dependent Biasing Models

M. Magliocchetti, J. S. Bagla, S. J. Maddox +1

We study the observed evolution of galaxy clustering as a function of redshift. We find that the clustering of galaxies decreases as we go from observations of the local Universe t…

astro-ph1997★ 54 cited

Evolution of Galaxy and Quasar Clustering

J. S. Bagla

We study the evolution of correlation function of dark matter halos in the CDM class of models. We show that the halo correlation function does not evolve in proportion with the co…

astro-ph1997

Gamma-ray bursts from stellar remnants: probing the Universe at high redshift

Ralph A. M. J. Wijers, Joshua S. Bloom, Jasjeet S. Bagla +1

A gamma-ray burst (GRB) releases an amount of energy similar to that of a supernova explosion, which combined with its rapid variability suggests an origin related to neutron stars…

astro-ph1997★ 29 cited

Clustering in Redshift Space at High Redshifts

J. S. Bagla

Recent observations show a large concentration of galaxies at high redshift. At first sight strong clustering of galaxies at high redshifts seems to be in contradiction with the mo…

astro-ph1996★ 49 cited

Critical Index and Fixed Point in the Transfer of Power in Nonlinear Gravitational Clustering

J. S. Bagla, T. Padmanabhan

We investigate the transfer of power between different scales and coupling of modes during non-linear evolution of gravitational clustering in an expanding universe. We start with…