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Title: A New Limit on CMB Circular Polarization from SPIDER

Journal Article · · The Astrophysical Journal (Online)
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  1. Case Western Reserve Univ., Cleveland, OH (United States). Physics Dept.
  2. Cardiff Univ., Cardiff (United Kingdom). School of Physics and Astronomy
  3. Univ. of British Columbia, Vancouver, BC (Canada). Dept. of Physics and Astronomy
  4. Princeton Univ., NJ (United States). Dept. of Physics
  5. 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.
  6. Univ. of Toronto, ON (Canada). Canadian Inst. for Theoretical Astrophysics
  7. Arizona State Univ., Tempe, AZ (United States). School of Earth and Space Exploration
  8. Univ. of KwaZulu-Natal, Durban (South Africa); National Institute for Theoretical Physics (NITheP), KwaZulu-Natal (South Africa)
  9. Imperial College, London (United Kingdom). Blackett Lab.
  10. Stockholm Univ. (Sweden). Oskar Klein Centre for Cosmoparticle Physics, Dept. of Physics
  11. Univ. of Oslo (Norway). Inst. of Theoretical Astrophysics
  12. Univ. of Toronto, ON (Canada). Canadian Inst. for Theoretical Astrophysics; Univ. of Toronto, ON (Canada). Dept. of Astronomy and Astrophysics
  13. Univ. of Illinois, Urbana-Champaign, IL (United States). Dept. of Physics; Univ. of Illinois, Urbana-Champaign, IL (United States). Dept. of Astronomy
  14. Univ. of Toronto, ON (Canada). Dept. of Astronomy and Astrophysics; National Radio Astronomy Observatory, Charlottesville, NC (United States)
  15. Stockholm Univ. (Sweden). Oskar Klein Centre for Cosmoparticle Physics, Dept. of Physics; Univ. of Michigan, Ann Arbor, MI (United States). Dept. of Physics
  16. Univ. of Toronto, ON (Canada). Dept. of Physics
  17. Johns Hopkins Univ., Baltimore, MD (United States). Department of Physics and Astronomy; NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
  18. Univ. Paris Diderot, Sorbonne Paris Cite (France)
  19. Pennsylvania State Univ., University Park, PA (United States). Dept of Astronomy and Astrophysics
  20. National Inst. of Standards and Technology (NIST), Boulder, CO (United States)
  21. California Inst. of Technology (CalTech), Pasadena, CA (United States). Jet Propulsion Lab.
  22. California Inst. of Technology (CalTech), Pasadena, CA (United States). Division of Physics, Mathematics and Astronomy
  23. Stanford Univ., CA (United States). Dept. of Physics; SLAC National Accelerator Lab., Menlo Park, CA (United States)
  24. SLAC National Accelerator Lab., Menlo Park, CA (United States)
  25. 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
  26. Univ. of Toronto, ON (Canada). Dept. of Astronomy and Astrophysics; Univ. of Toronto, ON (Canada). Dept. of Physics
  27. Univ. of Toronto, ON (Canada). Dept. of Astronomy and Astrophysics
  28. Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics
  29. 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
Citation Metrics:
Cited by: 35 works
Citation information provided by
Web of Science

References (24)

Generation of circular polarization of the cosmic microwave background journal March 2009
Modeling and characterization of the SPIDER half-wave plate conference July 2010
A cryogenic rotation stage with a large clear aperture for the half-wave plates in the Spider instrument journal January 2016
Modeling dielectric half-wave plates for cosmic microwave background polarimetry using a Mueller matrix formalism journal January 2010
Fast estimation of polarization power spectra using correlation functions journal May 2004
Lorentz-violating extension of the standard model journal October 1998
Is the cosmic microwave background circularly polarized? journal February 2003
Circular polarization of the CMB: A probe of the first stars journal December 2015
Rotation of linear polarization plane and circular polarization from cosmological pseudoscalar fields journal March 2009
V -mode polarization of the cosmic microwave background journal December 2009
The thermal design, characterization, and performance of the S pider long-duration balloon cryostat journal December 2015
Circular polarization of the CMB: Foregrounds and detection prospects journal July 2016
Miscellaneous data on materials for millimetre and submillimetre optics journal December 1996
Linear and circular polarization of the cosmic background radiation journal October 1983
Evidence for cosmic neutrino background from CMB circular polarization journal October 2014
Linear polarized fluctuations in the cosmic microwave background journal January 1988
Achromatic half-wave plate for submillimeter instruments in cosmic microwave background astronomy: experimental characterization journal January 2006
Planck 2015 results : X. Diffuse component separation: Foreground maps journal September 2016
Planck 2015 results : I. Overview of products and scientific results journal September 2016
Pre-flight integration and characterization of the SPIDER balloon-borne telescope conference July 2014
Recovering the frequency dependent modulation function of the achromatic half-wave plate for POL-2: the SCUBA-2 polarimeter journal January 2009
Achromatic half-wave plate for submillimeter instruments in cosmic microwave background astronomy: modeling and simulation journal January 2006
Photon-photon interactions as a source of cosmic microwave background circular polarization journal January 2015
Generation of circular polarization of the CMB journal April 2010

Cited By (15)

SPIDER: CMB Polarimetry from the Edge of Space journal October 2018
Balloon-borne Cosmic Microwave Background experiments journal January 2019
Probing large-scale magnetism with the cosmic microwave background journal March 2018
Using the full power of the cosmic microwave background to probe axion dark matter journal February 2018
Full-sky beam convolution for cosmic microwave background applications journal May 2019
Probing gravitational parity violation with gravitational waves from stellar-mass black hole binaries journal May 2018
Circular polarization in a spherical basis journal June 2018
Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: A Measurement of Circular Polarization at 40 GHz journal January 2020
Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: A First Detection of Atmospheric Circular Polarization at Q band journal January 2020
SPIDER: CMB polarimetry from the edge of space text January 2017
Probing Gravitational Parity Violation with Gravitational Waves from Stellar-mass Black Hole Binaries text January 2017
Probing large-scale magnetism with the Cosmic Microwave Background text January 2017
Axion Dark Matter Detection with CMB Polarization text January 2019
Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: A Measurement of Circular Polarization at 40 GHz text January 2019
Two-year Cosmology Large Angular Scale Surveyor (CLASS) Observations: A First Detection of Atmospheric Circular Polarization at Q Band text January 2019

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