A New Limit on CMB Circular Polarization from SPIDER
- Case Western Reserve Univ., Cleveland, OH (United States). Physics Dept.
- Cardiff Univ., Cardiff (United Kingdom). School of Physics and Astronomy
- Univ. of British Columbia, Vancouver, BC (Canada). Dept. of Physics and Astronomy
- Princeton Univ., NJ (United States). Dept. of Physics
- California Inst. of Technology (CalTech), Pasadena, CA (United States). Division of Physics, Mathematics and Astronomy; California Inst. of Technology (CalTech), Pasadena, CA (United States). Jet Propulsion Lab.
- Univ. of Toronto, ON (Canada). Canadian Inst. for Theoretical Astrophysics
- Arizona State Univ., Tempe, AZ (United States). School of Earth and Space Exploration
- Univ. of KwaZulu-Natal, Durban (South Africa); National Institute for Theoretical Physics (NITheP), KwaZulu-Natal (South Africa)
- Imperial College, London (United Kingdom). Blackett Lab.
- Stockholm Univ. (Sweden). Oskar Klein Centre for Cosmoparticle Physics, Dept. of Physics
- Univ. of Oslo (Norway). Inst. of Theoretical Astrophysics
- Univ. of Toronto, ON (Canada). Canadian Inst. for Theoretical Astrophysics; Univ. of Toronto, ON (Canada). Dept. of Astronomy and Astrophysics
- Univ. of Illinois, Urbana-Champaign, IL (United States). Dept. of Physics; Univ. of Illinois, Urbana-Champaign, IL (United States). Dept. of Astronomy
- Univ. of Toronto, ON (Canada). Dept. of Astronomy and Astrophysics; National Radio Astronomy Observatory, Charlottesville, NC (United States)
- Stockholm Univ. (Sweden). Oskar Klein Centre for Cosmoparticle Physics, Dept. of Physics; Univ. of Michigan, Ann Arbor, MI (United States). Dept. of Physics
- Univ. of Toronto, ON (Canada). Dept. of Physics
- Johns Hopkins Univ., Baltimore, MD (United States). Department of Physics and Astronomy; NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
- Univ. Paris Diderot, Sorbonne Paris Cite (France)
- Pennsylvania State Univ., University Park, PA (United States). Dept of Astronomy and Astrophysics
- National Inst. of Standards and Technology (NIST), Boulder, CO (United States)
- California Inst. of Technology (CalTech), Pasadena, CA (United States). Jet Propulsion Lab.
- California Inst. of Technology (CalTech), Pasadena, CA (United States). Division of Physics, Mathematics and Astronomy
- Stanford Univ., CA (United States). Dept. of Physics; SLAC National Accelerator Lab., Menlo Park, CA (United States)
- SLAC National Accelerator Lab., Menlo Park, CA (United States)
- Princeton Univ., NJ (United States). Dept. of Physics; Univ. of Toronto, ON (Canada). Dept. of Astronomy and Astrophysics; Princeton Univ., NJ (United States). Dept. of Mechanical and Aerospace Engineering
- Univ. of Toronto, ON (Canada). Dept. of Astronomy and Astrophysics; Univ. of Toronto, ON (Canada). Dept. of Physics
- Univ. of Toronto, ON (Canada). Dept. of Astronomy and Astrophysics
- Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics
- Max Planck Inst. for Astronomy, Heidelberg, (Germany); Astrophysics, Instrumentation and Modelling (AIM) Lab., Gif-sur-Yvette Cedex (France) ; Univ. Paris Diderot, Paris (France)
We present a new upper limit on CMB circular polarization from the 2015 flight of SPIDER, a balloon-borne telescope designed to search for $$B$$-mode linear polarization from cosmic inflation. Although the level of circular polarization in the CMB is predicted to be very small, experimental limits provide a valuable test of the underlying models. By exploiting the non-zero circular-to-linear polarization coupling of the HWP polarization modulators, data from SPIDER's 2015 Antarctic flight provides a constraint on Stokes $$V$$ at 95 and 150 GHz from $$33<\ell<307$$. No other limits exist over this full range of angular scales, and SPIDER improves upon the previous limit by several orders of magnitude, providing 95% C.L. constraints on $$\ell (\ell+1)C_{\ell}^{VV}/(2\pi)$$ ranging from 141 $$\mu K ^2$$ to 203 $$\mu K ^2$$ at 150 GHz for a thermal CMB spectrum. As linear CMB polarization experiments become increasingly sensitive, the techniques described in this paper can be applied to obtain stronger constraints on circular polarization.
- Research Organization:
- SLAC National Accelerator Lab., Menlo Park, CA (United States); Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
- Sponsoring Organization:
- USDOE Office of Science (SC), High Energy Physics (HEP)
- Contributing Organization:
- SPIDER
- Grant/Contract Number:
- AC02-76SF00515; AC02-07CH11359
- OSTI ID:
- 1390288
- Alternate ID(s):
- OSTI ID: 1362139
- Report Number(s):
- FERMILAB-PUB-17-135-AE; arXiv:1704.00215
- Journal Information:
- The Astrophysical Journal (Online), Vol. 844, Issue 2; ISSN 1538-4357
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
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