A New Limit on CMB Circular Polarization from SPIDER

J. M. Nagy; P. A.R. Ade; M. Amiri; S. J. Benton; A. S. Bergman; R. Bihary; J. J. Bock; J. R. Bond; S. A. Bryan; H. C. Chiang; C. R. Contaldi; O. Doré; A. J. Duivenvoorden; H. K. Eriksen; M. Farhang; J. P. Filippini; L. M. Fissel; A. A. Fraisse; K. Freese; M. Galloway; A. E. Gambrel; N. N. Gandilo; K. Ganga; J. E. Gudmundsson; M. Halpern; J. Hartley; M. Hasselfield; G. Hilton; W. Holmes; V. V. Hristov; Z. Huang; K. D. Irwin; W. C. Jones; C. L. Kuo; Z. D. Kermish; S. Li; P. V. Mason; K. Megerian; L. Moncelsi; T. A. Morford; C. B. Netterfield; M. Nolta; I. L. Padilla; B. Racine; A. S. Rahlin; C. Reintsema; J. E. Ruhl; M. C. Runyan; T. M. Ruud; J. A. Shariff; J. D. Soler; X. Song; A. Trangsrud; C. Tucker; R. S. Tucker; A. D. Turner; J. F.Van Der List; A. C. Weber; I. K. Wehus; D. V. Wiebe; E. Y. Young

doi:10.3847/1538-4357/aa7cfd

A New Limit on CMB Circular Polarization from SPIDER

J. M. Nagy, P. A.R. Ade, M. Amiri, S. J. Benton, A. S. Bergman, R. Bihary, J. J. Bock, J. R. Bond, S. A. Bryan, H. C. Chiang, C. R. Contaldi, O. Doré, A. J. Duivenvoorden, H. K. Eriksen, M. Farhang, J. P. Filippini, L. M. Fissel, A. A. Fraisse, K. Freese, M. GallowayA. E. Gambrel, N. N. Gandilo, K. Ganga, J. E. Gudmundsson, M. Halpern, J. Hartley, M. Hasselfield, G. Hilton, W. Holmes, V. V. Hristov, Z. Huang, K. D. Irwin, W. C. Jones, C. L. Kuo, Z. D. Kermish, S. Li, P. V. Mason, K. Megerian, L. Moncelsi, T. A. Morford, C. B. Netterfield, M. Nolta, I. L. Padilla, B. Racine, A. S. Rahlin, C. Reintsema, J. E. Ruhl, M. C. Runyan, T. M. Ruud, J. A. Shariff, J. D. Soler, X. Song, A. Trangsrud, C. Tucker, R. S. Tucker, A. D. Turner, J. F.Van Der List, A. C. Weber, I. K. Wehus, D. V. Wiebe, E. Y. Young

Earth and Space Exploration, School of (SESE)

Research output: Contribution to journal › Article › peer-review

43 Scopus citations

Abstract

We present a new upper limit on cosmic microwave background (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 nonzero circular-to-linear polarization coupling of the half-wave plate polarization modulators, data from Spider's 2015 Antarctic flight provide a constraint on Stokes V at 95 and 150 GHz in the range 33 < ℓ < 307. No other limits exist over this full range of angular scales, and Spider improves on the previous limit by several orders of magnitude, providing 95% C.L. constraints on ℓ( ℓ+1)C_t ^δV/2π ranging from 141 to 255 μK² 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 even stronger constraints on circular polarization.

Original language	English (US)
Article number	151
Journal	Astrophysical Journal
Volume	844
Issue number	2
DOIs	https://doi.org/10.3847/1538-4357/aa7cfd
State	Published - Aug 1 2017

Keywords

cosmic background radiation

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.3847/1538-4357/aa7cfd

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Nagy, J. M., Ade, P. A. R., Amiri, M., Benton, S. J., Bergman, A. S., Bihary, R., Bock, J. J., Bond, J. R., Bryan, S. A., Chiang, H. C., Contaldi, C. R., Doré, O., Duivenvoorden, A. J., Eriksen, H. K., Farhang, M., Filippini, J. P., Fissel, L. M., Fraisse, A. A., Freese, K., ... Young, E. Y. (2017). A New Limit on CMB Circular Polarization from SPIDER. Astrophysical Journal, 844(2), Article 151. https://doi.org/10.3847/1538-4357/aa7cfd

Nagy, JM, Ade, PAR, Amiri, M, Benton, SJ, Bergman, AS, Bihary, R, Bock, JJ, Bond, JR, Bryan, SA, Chiang, HC, Contaldi, CR, Doré, O, Duivenvoorden, AJ, Eriksen, HK, Farhang, M, Filippini, JP, Fissel, LM, Fraisse, AA, Freese, K, Galloway, M, Gambrel, AE, Gandilo, NN, Ganga, K, Gudmundsson, JE, Halpern, M, Hartley, J, Hasselfield, M, Hilton, G, Holmes, W, Hristov, VV, Huang, Z, Irwin, KD, Jones, WC, Kuo, CL, Kermish, ZD, Li, S, Mason, PV, Megerian, K, Moncelsi, L, Morford, TA, Netterfield, CB, Nolta, M, Padilla, IL, Racine, B, Rahlin, AS, Reintsema, C, Ruhl, JE, Runyan, MC, Ruud, TM, Shariff, JA, Soler, JD, Song, X, Trangsrud, A, Tucker, C, Tucker, RS, Turner, AD, List, JFVD, Weber, AC, Wehus, IK, Wiebe, DV & Young, EY 2017, 'A New Limit on CMB Circular Polarization from SPIDER', Astrophysical Journal, vol. 844, no. 2, 151. https://doi.org/10.3847/1538-4357/aa7cfd

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title = "A New Limit on CMB Circular Polarization from SPIDER",

abstract = "We present a new upper limit on cosmic microwave background (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 nonzero circular-to-linear polarization coupling of the half-wave plate polarization modulators, data from Spider's 2015 Antarctic flight provide a constraint on Stokes V at 95 and 150 GHz in the range 33 < ℓ < 307. No other limits exist over this full range of angular scales, and Spider improves on the previous limit by several orders of magnitude, providing 95% C.L. constraints on ℓ( ℓ+1)Ct δV/2π ranging from 141 to 255 μK2 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 even stronger constraints on circular polarization.",

keywords = "cosmic background radiation",

author = "Nagy, {J. M.} and Ade, {P. A.R.} and M. Amiri and Benton, {S. J.} and Bergman, {A. S.} and R. Bihary and Bock, {J. J.} and Bond, {J. R.} and Bryan, {S. A.} and Chiang, {H. C.} and Contaldi, {C. R.} and O. Dor{\'e} and Duivenvoorden, {A. J.} and Eriksen, {H. K.} and M. Farhang and Filippini, {J. P.} and Fissel, {L. M.} and Fraisse, {A. A.} and K. Freese and M. Galloway and Gambrel, {A. E.} and Gandilo, {N. N.} and K. Ganga and Gudmundsson, {J. E.} and M. Halpern and J. Hartley and M. Hasselfield and G. Hilton and W. Holmes and Hristov, {V. V.} and Z. Huang and Irwin, {K. D.} and Jones, {W. C.} and Kuo, {C. L.} and Kermish, {Z. D.} and S. Li and Mason, {P. V.} and K. Megerian and L. Moncelsi and Morford, {T. A.} and Netterfield, {C. B.} and M. Nolta and Padilla, {I. L.} and B. Racine and Rahlin, {A. S.} and C. Reintsema and Ruhl, {J. E.} and Runyan, {M. C.} and Ruud, {T. M.} and Shariff, {J. A.} and Soler, {J. D.} and X. Song and A. Trangsrud and C. Tucker and Tucker, {R. S.} and Turner, {A. D.} and List, {J. F.Van Der} and Weber, {A. C.} and Wehus, {I. K.} and Wiebe, {D. V.} and Young, {E. Y.}",

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doi = "10.3847/1538-4357/aa7cfd",

language = "English (US)",

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journal = "Astrophysical Journal",

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T1 - A New Limit on CMB Circular Polarization from SPIDER

AU - Nagy, J. M.

AU - Ade, P. A.R.

AU - Amiri, M.

AU - Benton, S. J.

AU - Bergman, A. S.

AU - Bihary, R.

AU - Bock, J. J.

AU - Bond, J. R.

AU - Bryan, S. A.

AU - Chiang, H. C.

AU - Contaldi, C. R.

AU - Doré, O.

AU - Duivenvoorden, A. J.

AU - Eriksen, H. K.

AU - Farhang, M.

AU - Filippini, J. P.

AU - Fissel, L. M.

AU - Fraisse, A. A.

AU - Freese, K.

AU - Galloway, M.

AU - Gambrel, A. E.

AU - Gandilo, N. N.

AU - Ganga, K.

AU - Gudmundsson, J. E.

AU - Halpern, M.

AU - Hartley, J.

AU - Hasselfield, M.

AU - Hilton, G.

AU - Holmes, W.

AU - Hristov, V. V.

AU - Huang, Z.

AU - Irwin, K. D.

AU - Jones, W. C.

AU - Kuo, C. L.

AU - Kermish, Z. D.

AU - Li, S.

AU - Mason, P. V.

AU - Megerian, K.

AU - Moncelsi, L.

AU - Morford, T. A.

AU - Netterfield, C. B.

AU - Nolta, M.

AU - Padilla, I. L.

AU - Racine, B.

AU - Rahlin, A. S.

AU - Reintsema, C.

AU - Ruhl, J. E.

AU - Runyan, M. C.

AU - Ruud, T. M.

AU - Shariff, J. A.

AU - Soler, J. D.

AU - Song, X.

AU - Trangsrud, A.

AU - Tucker, C.

AU - Tucker, R. S.

AU - Turner, A. D.

AU - List, J. F.Van Der

AU - Weber, A. C.

AU - Wehus, I. K.

AU - Wiebe, D. V.

AU - Young, E. Y.

PY - 2017/8/1

Y1 - 2017/8/1

N2 - We present a new upper limit on cosmic microwave background (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 nonzero circular-to-linear polarization coupling of the half-wave plate polarization modulators, data from Spider's 2015 Antarctic flight provide a constraint on Stokes V at 95 and 150 GHz in the range 33 < ℓ < 307. No other limits exist over this full range of angular scales, and Spider improves on the previous limit by several orders of magnitude, providing 95% C.L. constraints on ℓ( ℓ+1)Ct δV/2π ranging from 141 to 255 μK2 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 even stronger constraints on circular polarization.

AB - We present a new upper limit on cosmic microwave background (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 nonzero circular-to-linear polarization coupling of the half-wave plate polarization modulators, data from Spider's 2015 Antarctic flight provide a constraint on Stokes V at 95 and 150 GHz in the range 33 < ℓ < 307. No other limits exist over this full range of angular scales, and Spider improves on the previous limit by several orders of magnitude, providing 95% C.L. constraints on ℓ( ℓ+1)Ct δV/2π ranging from 141 to 255 μK2 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 even stronger constraints on circular polarization.

KW - cosmic background radiation

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UR - http://www.scopus.com/inward/citedby.url?scp=85027295154&partnerID=8YFLogxK

U2 - 10.3847/1538-4357/aa7cfd

DO - 10.3847/1538-4357/aa7cfd

M3 - Article

AN - SCOPUS:85027295154

SN - 0004-637X

VL - 844

JO - Astrophysical Journal

JF - Astrophysical Journal

IS - 2

M1 - 151

ER -

A New Limit on CMB Circular Polarization from SPIDER

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