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H i as a probe of the large-scale structure in the post-reionization universe

Monthly notices of the Royal Astronomical Society, 2010-09, Vol.407 (1), p.567-580

2010

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Non-linear spherical collapse in tachyon models and a comparison of collapse in tachyon and quintessence models of dark energy

Classical and quantum gravity, 2020-12, Vol.37 (23), p.235008

2020

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Fractal dimension as a measure of the scale of homogeneity

Monthly notices of the Royal Astronomical Society, 2010-07, Vol.405 (3), p.2009-2015

2010

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Understanding the origin of CMB constraints on dark energy

Monthly notices of the Royal Astronomical Society, 2010-07, Vol.405 (4), p.2639-2650

2010

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The Adaptive TreePM: an adaptive resolution code for cosmological N-body simulations

Monthly notices of the Royal Astronomical Society, 2009-07, Vol.396 (4), p.2211-2227

2009

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Fractal dimensions of a weakly clustered distribution and the scale of homogeneity

Monthly notices of the Royal Astronomical Society, 2008-10, Vol.390 (2), p.829-838

2008

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

Monthly notices of the Royal Astronomical Society, 2009-02, Vol.393 (2), p.607-614

2009

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Finding singularities in gravitational lensing

Monthly notices of the Royal Astronomical Society, 2020-03, Vol.492 (3), p.3294-3305

2020

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

Monthly notices of the Royal Astronomical Society, 2005-04, Vol.358 (3), p.1076-1082

2005

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Cosmological N-body simulation: Techniques, scope and status

Current science (Bangalore), 2005-04, Vol.88 (7), p.1088-1100

Bagla, J. S.

2005

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Effects of the size of cosmological N-body simulations on physical quantities – III. Skewness

Monthly notices of the Royal Astronomical Society, 2009-05, Vol.395 (2), p.918-930

2009

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Effects of the size of cosmological N-body simulations on physical quantities - I. Mass function

Monthly notices of the Royal Astronomical Society, 2006-08, Vol.370 (2), p.993-1002

2006

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Metal enrichment and reionization constraints on early star formation

Monthly notices of the Royal Astronomical Society, 2009-08, Vol.397 (2), p.971-978

2009

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Cecilia Payne-Gaposchkin

Resonance, 2022, Vol.27 (11), p.1835-1836

Bagla, J. S.

2022

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Tachyonic vs quintessence dark energy: linear perturbations and CMB data

Classical and quantum gravity, 2021-10, Vol.38 (19), p.195001

2021

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Reconstruction of dynamical dark energy potentials: Quintessence, tachyon and interacting models

Journal of astrophysics and astronomy, 2019-12, Vol.40 (6), p.1-9, Article 44

2019

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

Monthly notices of the Royal Astronomical Society, 1998-02, Vol.294 (1), p.L13-L17

1998

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A modified TreePM code

Chinese journal of astronomy and astrophysics, 2009-08, Vol.9 (8), p.861-873

2009

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WMAP constraints on low redshift evolution of dark energy

Monthly notices of the Royal Astronomical Society. Letters, 2005-01, Vol.356 (1), p.L11-L16

2005

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Cosmology with tachyon field as dark energy

Physical review. D, Particles and fields, 2003-03, Vol.67 (6), Article 063504

2003

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

Monthly notices of the Royal Astronomical Society, 2005-06, Vol.360 (1), p.194-202

2005

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TreePM: A code for cosmological N-body simulations

Journal of astrophysics and astronomy, 2002-12, Vol.23 (3-4), p.185-196

Bagla, JS

2002

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Gravitational collapse in an expanding universe: scaling relations for two-dimensional collapse revisited

Monthly notices of the Royal Astronomical Society, 2005-06, Vol.360 (2), p.546-554

2005

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Gravitational Collapse and Structure Formation in an Expanding Universe with Dark Energy

Resonance, 2019-09, Vol.24 (9), p.977-993

2019

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Evolution of galaxy clustering

Monthly notices of the Royal Astronomical Society, 1998-09, Vol.299 (2), p.417-424

Bagla, J. S.

1998

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H i as a probe of the large-scale structure in the post-reionization universe

Non-linear spherical collapse in tachyon models and a comparison of collapse in tachyon and quintessence models of dark energy

Fractal dimension as a measure of the scale of homogeneity

Understanding the origin of CMB constraints on dark energy

The Adaptive TreePM: an adaptive resolution code for cosmological N-body simulations

Fractal dimensions of a weakly clustered distribution and the scale of homogeneity

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

Finding singularities in gravitational lensing

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

Cosmological N-body simulation: Techniques, scope and status

Effects of the size of cosmological N-body simulations on physical quantities – III. Skewness

Effects of the size of cosmological N-body simulations on physical quantities - I. Mass function

Metal enrichment and reionization constraints on early star formation

Cecilia Payne-Gaposchkin

Tachyonic vs quintessence dark energy: linear perturbations and CMB data

Reconstruction of dynamical dark energy potentials: Quintessence, tachyon and interacting models

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

A modified TreePM code

WMAP constraints on low redshift evolution of dark energy

Cosmology with tachyon field as dark energy

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

TreePM: A code for cosmological N-body simulations

Gravitational collapse in an expanding universe: scaling relations for two-dimensional collapse revisited

Gravitational Collapse and Structure Formation in an Expanding Universe with Dark Energy

Evolution of galaxy clustering

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