Fitting the nonlinear matter bispectrum by the Halofit approach

التفاصيل البيبلوغرافية
العنوان: Fitting the nonlinear matter bispectrum by the Halofit approach
المؤلفون: Atsushi Taruya, Masato Shirasaki, Issha Kayo, Yosuke Kobayashi, Toshiya Namikawa, Takahiro Nishimichi, Ryuichi Takahashi, Ken Osato
المساهمون: Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
المصدر: Astrophys.J.
Astrophys.J., 2020, 895 (2), pp.113. ⟨10.3847/1538-4357/ab908d⟩
سنة النشر: 2019
مصطلحات موضوعية: Cosmology and Nongalactic Astrophysics (astro-ph.CO), Cold dark matter, 010504 meteorology & atmospheric sciences, Cosmic microwave background, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), Astrophysics::Cosmology and Extragalactic Astrophysics, 01 natural sciences, General Relativity and Quantum Cosmology, symbols.namesake, 0103 physical sciences, Sample variance, Planck, 010303 astronomy & astrophysics, Weak gravitational lensing, 0105 earth and related environmental sciences, Mathematical physics, Physics, Astronomy and Astrophysics, Redshift, Cover (topology), Space and Planetary Science, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], symbols, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], Bispectrum, Astrophysics - Cosmology and Nongalactic Astrophysics
الوصف: We provide a new fitting formula of the matter bispectrum in the nonlinear regime calibrated by high-resolution cosmological $N$-body simulations of $41$ cold dark matter ($w$CDM, $w=$ constant) models around the Planck 2015 best-fit parameters. As the parameterization in our fitting function is similar to that in Halofit, our fitting is named BiHalofit. The simulation volume is sufficiently large ($> 10 \, {\rm Gpc}^3$) to cover almost all measurable triangle bispectrum configurations in the universe. The function is also calibrated using one-loop perturbation theory at large scales ($k
23 pages, 15 figures; accepted for publication in ApJ; typos corrected; numerical codes of the fitting formula are available at https://toshiyan.github.io/clpdoc/html/basic/basic.html#module-basic.bispec (Python) and http://cosmo.phys.hirosaki-u.ac.jp/takahasi/codes_e.htm (C and Fortran)
اللغة: English
URL الوصول: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::298fcebb032f8173caa8325ec982f4f0
http://arxiv.org/abs/1911.07886
حقوق: OPEN
رقم الأكسشن: edsair.doi.dedup.....298fcebb032f8173caa8325ec982f4f0
قاعدة البيانات: OpenAIRE