کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
5494327 | 1527703 | 2017 | 17 صفحه PDF | دانلود رایگان |
عنوان انگلیسی مقاله ISI
Constraining the ionized gas evolution with CMB-spectroscopic survey cross-correlation
دانلود مقاله + سفارش ترجمه
دانلود مقاله ISI انگلیسی
رایگان برای ایرانیان
موضوعات مرتبط
مهندسی و علوم پایه
ریاضیات
فیزیک ریاضی
پیش نمایش صفحه اول مقاله
چکیده انگلیسی
We forecast the prospective constraints on the ionized gas model fgas(z) at different evolutionary epochs via the tomographic cross-correlation between kinetic Sunyaev-Zeldovich (kSZ) effect and the reconstructed momentum field at different redshifts. The experiments we consider are the Planck and CMB Stage-4 survey for CMB and the SDSS-III for the galaxy spectroscopic survey. We calculate the tomographic cross-correlation power spectrum, and use the Fisher matrix to forecast the detectability of different fgas(z) models. We find that for constant fgas model, Planck can constrain the error of fgas (Ïfgas) at each redshift bin to â¼0.2, whereas four cases of CMB-S4 can achieve Ïfgasâ¼10â3. For fgas(z)=fgas,0/(1+z) model the error budget will be slightly broadened. We also investigate the model fgas(z)=fgas,0/(1+z)α. Planck is unable to constrain the index of redshift evolution, but the CMB-S4 experiments can constrain the index α to the level of Ïαâ¼0.01-0.1. The tomographic cross-correlation method will provide an accurate measurement of the ionized gas evolution at different epochs of the Universe.
ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Nuclear Physics B - Volume 920, July 2017, Pages 402-418
Journal: Nuclear Physics B - Volume 920, July 2017, Pages 402-418
نویسندگان
Yin-Zhe Ma,