activity
20042008
most citedLines in the Cosmic Microwave Background Spectrum from the Epoch of Cosmological Hydrogen Recombination

110 citations · 604 across the 11 of their papers we have counts for

collaborators

13 papers

astro-ph200831 cited

Time-Dependent Corrections to the Ly-alpha Escape Probability During Cosmological Hydrogen Recombination

J. Chluba, R. A. Sunyaev

We consider the effects connected with the detailed radiative transfer during the epoch of cosmological recombination on the ionization history of our Universe. We focus on the esc…

astro-ph200819 cited

Evolution of low-frequency features in the CMB spectrum due to stimulated Compton scattering and Doppler-broadening

J. Chluba, R. A. Sunyaev

We discuss a new solution of the Kompaneets-equation for physical situations in which low frequency photons, forming relatively narrow spectral details, are Compton scattered in an…

astro-ph200795 cited

Lines in the cosmic microwave background spectrum from the epoch of cosmological helium recombination

J. A. Rubino-Martin, J. Chluba, R. A. Sunyaev

The main goal of this work is to calculate the contributions to the cosmological recombination spectrum due to bound-bound transitions of helium. We show that due to the presence o…

astro-ph2007

The Richness and Beauty of the Physics of Cosmological Recombination

R. A. Sunyaev, J. Chluba

The physical ingredients to describe the epoch of cosmological recombination are amazingly simple and well-understood. This fact allows us to take into account a very large variety…

astro-ph200743 cited

Is there a need and another way to measure the Cosmic Microwave Background temperature more accurately?

J. Chluba, R. A. Sunyaev

The recombination history of the Universe depends exponentially on the temperature, T_0, of the cosmic microwave background. Therefore tiny changes of T_0 are expected to lead to s…

astro-ph200775 cited

Two-photon transitions in hydrogen and cosmological recombination

J. Chluba, R. A. Sunyaev

We study the two-photon process for the transitions ns --> 1s and nd --> 1s in hydrogen up to large n. For n<=20 we provide simple analytic fitting formulae to describe the non-res…