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A New method of measuring the peculiar velocity power spectrum

Journal Article · · TBD
OSTI ID:1864216
We show that by directly correlating the cluster kinetic Sunyaev Zeldovich (KSZ) flux, the cluster peculiar velocity power spectrum can be measured to $$\sim 10%$$ accuracy by future large sky coverage KSZ surveys. This method is almost free of systemics entangled in the usual velocity inversion method. The direct correlation brings extra information of density and velocity clustering. We utilize these information to construct two indicators of the Hubble constant and comoving angular distance and propose a novel method to constrain cosmology.
Research Organization:
Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25)
DOE Contract Number:
AC02-07CH11359
OSTI ID:
1864216
Report Number(s):
FERMILAB-PUB-04-304-A; arXiv:astro-ph/0410637; oai:inspirehep.net:662821
Journal Information:
TBD, Journal Name: TBD
Country of Publication:
United States
Language:
English

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