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Matter bispectrum of large-scale structure: Three-dimensional comparison between theoretical models and numerical simulations

Physical review. D, 2016-04, Vol.93 (8), Article 083517

2016

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Polyspectra searches for sharp oscillatory features in cosmic microwave sky data

Physical review. D, Particles, fields, gravitation, and cosmology, 2015-06, Vol.91 (12), Article 123506

2015

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Combining power spectrum and bispectrum measurements to detect oscillatory features

Physical review. D, Particles, fields, gravitation, and cosmology, 2015-01, Vol.91 (2), Article 023502

2015

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Using inpainting to construct accurate cut-sky CMB estimators

Physical review. D, 2017-02, Vol.95 (4), Article 043532

2017

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Generalized velocity-dependent one-scale model for current-carrying strings

Physical review. D, 2021-02, Vol.103 (4), Article 043538

2021

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Matter bispectrum of large-scale structure with Gaussian and non-Gaussian initial conditions: Halo models, perturbation theory, and a three-shape model

Physical review. D, 2017-04, Vol.95 (8), Article 083511

2017

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Extending the velocity-dependent one-scale model for domain walls

Physical review. D, 2016-02, Vol.93 (4), Article 043534

2016

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Primordial Non-Gaussianity and Bispectrum Measurements in the Cosmic Microwave Background and Large-Scale Structure

Advances in Astronomy, 2010-01, Vol.2010 (1), p.1101-1164

2010

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Stretching and Kibble scaling regimes for Hubble-damped defect networks

Physical review. D, 2016-12, Vol.94 (11), Article 116017

2016

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Models for small-scale structure on cosmic strings. II. Scaling and its stability

Physical review. D, 2016-11, Vol.94 (9), Article 096005

2016

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High-resolution CMB bispectrum estimator with flexible modal bases

Physical review. D, 2023-09, Vol.108 (6), Article 063504

2023

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Radiation from global topological strings using adaptive mesh refinement: Methodology and massless modes

Physical review. D, 2022-03, Vol.105 (6), Article 063517

2022

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Radiation from global topological strings using adaptive mesh refinement: Massive modes

Physical review. D, 2023-02, Vol.107 (4), Article 043507

2023

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Editorial Note: Models for small-scale structure on cosmic strings. II. Scaling and its stability [Phys. Rev. D 94 , 096005 (2016)]

Physical review. D, 2016-11, Vol.94 (9), Article 099907

2016

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Charge-velocity-dependent one-scale linear model

Physical review. D, 2021-11, Vol.104 (10), Article 103506

2021

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Rapid separable analysis of higher order correlators in large-scale structure

Physical review. D, Particles, fields, gravitation, and cosmology, 2012-09, Vol.86 (6), Article 063511

2012

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Fast estimation of gravitational and primordial bispectra in large scale structures

Physical review. D, Particles, fields, gravitation, and cosmology, 2013-09, Vol.88 (6), Article 063512

2013

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Effects and detectability of quasi-single field inflation in the large-scale structure and cosmic microwave background

Journal of cosmology and astroparticle physics, 2012-08, Vol.2012 (8), p.33-33

2012

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Fractal properties and small-scale structure of cosmic string networks

Physical review. D, Particles, fields, gravitation, and cosmology, 2006-02, Vol.73 (4), Article 043515

2006

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The CMB bispectrum

Journal of cosmology and astroparticle physics, 2012-12, Vol.2012 (12), p.32-32

2012

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Unified model for vortex-string network evolution

Physical review letters, 2004-06, Vol.92 (25), p.251601.1-251601.4, Article 251601

2004

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Extending the velocity-dependent one-scale string evolution model

Physical review. D, Particles and fields, 2002, Vol.65 (4), Article 043514

2002

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Cosmic-string evolution: a numerical simulation

Physical review letters, 1990-01, Vol.64 (2), p.119-122

1990

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Separate universe approach and the evolution of nonlinear superhorizon cosmological perturbations

Physical review. D, Particles and fields, 2003-12, Vol.68 (12), Article 123518

2003

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Universal non-Gaussian initial conditions for N -body simulations

Physical review. D, Particles, fields, gravitation, and cosmology, 2012-12, Vol.86 (12), Article 123524

2012

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Matter bispectrum of large-scale structure: Three-dimensional comparison between theoretical models and numerical simulations

Polyspectra searches for sharp oscillatory features in cosmic microwave sky data

Combining power spectrum and bispectrum measurements to detect oscillatory features

Using inpainting to construct accurate cut-sky CMB estimators

Generalized velocity-dependent one-scale model for current-carrying strings

Matter bispectrum of large-scale structure with Gaussian and non-Gaussian initial conditions: Halo models, perturbation theory, and a three-shape model

Extending the velocity-dependent one-scale model for domain walls

Primordial Non-Gaussianity and Bispectrum Measurements in the Cosmic Microwave Background and Large-Scale Structure

Stretching and Kibble scaling regimes for Hubble-damped defect networks

Models for small-scale structure on cosmic strings. II. Scaling and its stability

High-resolution CMB bispectrum estimator with flexible modal bases

Radiation from global topological strings using adaptive mesh refinement: Methodology and massless modes

Radiation from global topological strings using adaptive mesh refinement: Massive modes

Editorial Note: Models for small-scale structure on cosmic strings. II. Scaling and its stability [Phys. Rev. D 94 , 096005 (2016)]

Charge-velocity-dependent one-scale linear model

Rapid separable analysis of higher order correlators in large-scale structure

Fast estimation of gravitational and primordial bispectra in large scale structures

Effects and detectability of quasi-single field inflation in the large-scale structure and cosmic microwave background

Fractal properties and small-scale structure of cosmic string networks

The CMB bispectrum

Unified model for vortex-string network evolution

Extending the velocity-dependent one-scale string evolution model

Cosmic-string evolution: a numerical simulation

Separate universe approach and the evolution of nonlinear superhorizon cosmological perturbations

Universal non-Gaussian initial conditions for N -body simulations

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