Search Results for author: Christopher M. Hirata

Found 5 papers, 3 papers with code

Small-scale structure and the Lyman-$α$ forest baryon acoustic oscillation feature

1 code implementation11 Jul 2017 Christopher M. Hirata

A key advantage of the BAO as a standard ruler is that it is a sharp feature and hence is more robust against broadband systematic effects than other cosmological probes.

Cosmology and Nongalactic Astrophysics

FAST-PT II: an algorithm to calculate convolution integrals of general tensor quantities in cosmological perturbation theory

2 code implementations20 Sep 2016 Xiao Fang, Jonathan A. Blazek, Joseph E. McEwen, Christopher M. Hirata

Cosmological perturbation theory is a powerful tool to predict the statistics of large-scale structure in the weakly non-linear regime, but even at 1-loop order it results in computationally expensive mode-coupling integrals.

Cosmology and Nongalactic Astrophysics

FAST-PT: a novel algorithm to calculate convolution integrals in cosmological perturbation theory

2 code implementations15 Mar 2016 Joseph E. McEwen, Xiao Fang, Christopher M. Hirata, Jonathan A. Blazek

We present a novel algorithm, FAST-PT, for performing convolution or mode-coupling integrals that appear in nonlinear cosmological perturbation theory.

Cosmology and Nongalactic Astrophysics

Wouthuysen-Field coupling strength and application to high-redshift 21 cm radiation

no code implementations5 Jul 2005 Christopher M. Hirata

(3) The spin-flip scatterings change the frequency of the photon and cause the photon spectrum to relax not to the kinetic temperature of the gas but to a temperature between the kinetic and spin temperatures, effectively reducing the strength of the Wouthuysen-Field coupling.

astro-ph

Intrinsic alignment-lensing interference as a contaminant of cosmic shear

no code implementations10 Jun 2004 Christopher M. Hirata, Uros Seljak

The first model predicts a gravitational-intrinsic (GI) correlation that can be much greater than the intrinsic-intrinsic (II) correlation for broad redshift distributions, and that remains when galaxies pairs at similar redshifts are rejected.

astro-ph

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