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Title: BICEP/ K e c k XIV: Improved constraints on axionlike polarization oscillations in the cosmic microwave background

Abstract

We present an improved search for axionlike polarization oscillations in the cosmic microwave background (CMB) with observations from the Keck Array. An all-sky, temporally sinusoidal rotation of CMB polarization, equivalent to a time-variable cosmic birefringence, is an observable manifestation of a local axion field and potentially allows a CMB polarimeter to detect axionlike dark matter directly. We describe improvements to the method presented in previous work, and we demonstrate the updated method with an expanded dataset consisting of the 2012–2015 observing seasons. We set limits on the axion-photon coupling constant for mass m in the range 10 - 23 10 - 18 eV , which corresponds to oscillation periods on the order of hours to years. Our results are consistent with the background model. For periods between 1 and 30 d ( 1.6×10 - 21 m4.8×10 - 20 eV ), the 95%-confidence upper limits on rotation amplitude are approximately constant with a median of 0.27°, which constrains the axion-photon coupling constant to g φ γ < ( 4.5 × 10 - 12 GeV - 1 ) m / ( 10 - 21 eV ) , if axionlike particles constitute all of the dark matter. More than half of the collected BICEP dataset has yet to be analyzed, and several current and future CMB polarimetry experiments can apply the methods presented here to achieve comparable or superior constraints. In the coming years, oscillation measurements can achieve the sensitivity to rule out unexplored regions of the axion parameter space.

Authors:
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Publication Date:
Research Org.:
SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
Sponsoring Org.:
USDOE
Contributing Org.:
BICEP/Keck Collaboration
OSTI Identifier:
1861995
Grant/Contract Number:  
AC02-76SF00515
Resource Type:
Accepted Manuscript
Journal Name:
Physical Review. D.
Additional Journal Information:
Journal Volume: 105; Journal Issue: 2; Journal ID: ISSN 2470-0010
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Cosmic microwave background; Dark matter; Axions

Citation Formats

Ade, P.  A. R., Ahmed, Z., Amiri, M., Barkats, D., Basu Thakur, R., Bischoff, C.  A., Beck, D., Bock, J.  J., Boenish, H., Bullock, E., Buza, V., Cheshire, J.  R., Connors, J., Cornelison, J., Crumrine, M., Cukierman, A., Denison, E.  V., Dierickx, M., Duband, L., Eiben, M., Fatigoni, S., Filippini, J.  P., Fliescher, S., Goeckner-Wald, N., Goldfinger, D.  C., Grayson, J., Grimes, P., Hall, G., Halal, G., Halpern, M., Hand, E., Harrison, S., Henderson, S., Hildebrandt, S.  R., Hilton, G.  C., Hubmayr, J., Hui, H., Irwin, K.  D., Kang, J., Karkare, K.  S., Karpel, E., Kefeli, S., Kernasovskiy, S.  A., Kovac, J.  M., Kuo, C.  L., Lau, K., Leitch, E.  M., Lennox, A., Megerian, K.  G., Minutolo, L., Moncelsi, L., Nakato, Y., Namikawa, T., Nguyen, H.  T., O’Brient, R., Ogburn, R.  W., Palladino, S., Prouve, T., Pryke, C., Racine, B., Reintsema, C.  D., Richter, S., Schillaci, A., Schwarz, R., Schmitt, B.  L., Sheehy, C.  D., Soliman, A., Germaine, T.  St., Steinbach, B., Sudiwala, R.  V., Teply, G.  P., Thompson, K.  L., Tolan, J.  E., Tucker, C., Turner, A.  D., Umiltà, C., Vergès, C., Vieregg, A.  G., Wandui, A., Weber, A.  C., Wiebe, D.  V., Willmert, J., Wong, C.  L., Wu, W.  L. K., Yang, H., Yoon, K.  W., Young, E., Yu, C., Zeng, L., Zhang, C., and Zhang, S. BICEP/Keck XIV: Improved constraints on axionlike polarization oscillations in the cosmic microwave background. United States: N. p., 2022. Web. doi:10.1103/physrevd.105.022006.
Ade, P.  A. R., Ahmed, Z., Amiri, M., Barkats, D., Basu Thakur, R., Bischoff, C.  A., Beck, D., Bock, J.  J., Boenish, H., Bullock, E., Buza, V., Cheshire, J.  R., Connors, J., Cornelison, J., Crumrine, M., Cukierman, A., Denison, E.  V., Dierickx, M., Duband, L., Eiben, M., Fatigoni, S., Filippini, J.  P., Fliescher, S., Goeckner-Wald, N., Goldfinger, D.  C., Grayson, J., Grimes, P., Hall, G., Halal, G., Halpern, M., Hand, E., Harrison, S., Henderson, S., Hildebrandt, S.  R., Hilton, G.  C., Hubmayr, J., Hui, H., Irwin, K.  D., Kang, J., Karkare, K.  S., Karpel, E., Kefeli, S., Kernasovskiy, S.  A., Kovac, J.  M., Kuo, C.  L., Lau, K., Leitch, E.  M., Lennox, A., Megerian, K.  G., Minutolo, L., Moncelsi, L., Nakato, Y., Namikawa, T., Nguyen, H.  T., O’Brient, R., Ogburn, R.  W., Palladino, S., Prouve, T., Pryke, C., Racine, B., Reintsema, C.  D., Richter, S., Schillaci, A., Schwarz, R., Schmitt, B.  L., Sheehy, C.  D., Soliman, A., Germaine, T.  St., Steinbach, B., Sudiwala, R.  V., Teply, G.  P., Thompson, K.  L., Tolan, J.  E., Tucker, C., Turner, A.  D., Umiltà, C., Vergès, C., Vieregg, A.  G., Wandui, A., Weber, A.  C., Wiebe, D.  V., Willmert, J., Wong, C.  L., Wu, W.  L. K., Yang, H., Yoon, K.  W., Young, E., Yu, C., Zeng, L., Zhang, C., & Zhang, S. BICEP/Keck XIV: Improved constraints on axionlike polarization oscillations in the cosmic microwave background. United States. https://doi.org/10.1103/physrevd.105.022006
Ade, P.  A. R., Ahmed, Z., Amiri, M., Barkats, D., Basu Thakur, R., Bischoff, C.  A., Beck, D., Bock, J.  J., Boenish, H., Bullock, E., Buza, V., Cheshire, J.  R., Connors, J., Cornelison, J., Crumrine, M., Cukierman, A., Denison, E.  V., Dierickx, M., Duband, L., Eiben, M., Fatigoni, S., Filippini, J.  P., Fliescher, S., Goeckner-Wald, N., Goldfinger, D.  C., Grayson, J., Grimes, P., Hall, G., Halal, G., Halpern, M., Hand, E., Harrison, S., Henderson, S., Hildebrandt, S.  R., Hilton, G.  C., Hubmayr, J., Hui, H., Irwin, K.  D., Kang, J., Karkare, K.  S., Karpel, E., Kefeli, S., Kernasovskiy, S.  A., Kovac, J.  M., Kuo, C.  L., Lau, K., Leitch, E.  M., Lennox, A., Megerian, K.  G., Minutolo, L., Moncelsi, L., Nakato, Y., Namikawa, T., Nguyen, H.  T., O’Brient, R., Ogburn, R.  W., Palladino, S., Prouve, T., Pryke, C., Racine, B., Reintsema, C.  D., Richter, S., Schillaci, A., Schwarz, R., Schmitt, B.  L., Sheehy, C.  D., Soliman, A., Germaine, T.  St., Steinbach, B., Sudiwala, R.  V., Teply, G.  P., Thompson, K.  L., Tolan, J.  E., Tucker, C., Turner, A.  D., Umiltà, C., Vergès, C., Vieregg, A.  G., Wandui, A., Weber, A.  C., Wiebe, D.  V., Willmert, J., Wong, C.  L., Wu, W.  L. K., Yang, H., Yoon, K.  W., Young, E., Yu, C., Zeng, L., Zhang, C., and Zhang, S. Fri . "BICEP/Keck XIV: Improved constraints on axionlike polarization oscillations in the cosmic microwave background". United States. https://doi.org/10.1103/physrevd.105.022006. https://www.osti.gov/servlets/purl/1861995.
@article{osti_1861995,
title = {BICEP/Keck XIV: Improved constraints on axionlike polarization oscillations in the cosmic microwave background},
author = {Ade, P.  A. R. and Ahmed, Z. and Amiri, M. and Barkats, D. and Basu Thakur, R. and Bischoff, C.  A. and Beck, D. and Bock, J.  J. and Boenish, H. and Bullock, E. and Buza, V. and Cheshire, J.  R. and Connors, J. and Cornelison, J. and Crumrine, M. and Cukierman, A. and Denison, E.  V. and Dierickx, M. and Duband, L. and Eiben, M. and Fatigoni, S. and Filippini, J.  P. and Fliescher, S. and Goeckner-Wald, N. and Goldfinger, D.  C. and Grayson, J. and Grimes, P. and Hall, G. and Halal, G. and Halpern, M. and Hand, E. and Harrison, S. and Henderson, S. and Hildebrandt, S.  R. and Hilton, G.  C. and Hubmayr, J. and Hui, H. and Irwin, K.  D. and Kang, J. and Karkare, K.  S. and Karpel, E. and Kefeli, S. and Kernasovskiy, S.  A. and Kovac, J.  M. and Kuo, C.  L. and Lau, K. and Leitch, E.  M. and Lennox, A. and Megerian, K.  G. and Minutolo, L. and Moncelsi, L. and Nakato, Y. and Namikawa, T. and Nguyen, H.  T. and O’Brient, R. and Ogburn, R.  W. and Palladino, S. and Prouve, T. and Pryke, C. and Racine, B. and Reintsema, C.  D. and Richter, S. and Schillaci, A. and Schwarz, R. and Schmitt, B.  L. and Sheehy, C.  D. and Soliman, A. and Germaine, T.  St. and Steinbach, B. and Sudiwala, R.  V. and Teply, G.  P. and Thompson, K.  L. and Tolan, J.  E. and Tucker, C. and Turner, A.  D. and Umiltà, C. and Vergès, C. and Vieregg, A.  G. and Wandui, A. and Weber, A.  C. and Wiebe, D.  V. and Willmert, J. and Wong, C.  L. and Wu, W.  L. K. and Yang, H. and Yoon, K.  W. and Young, E. and Yu, C. and Zeng, L. and Zhang, C. and Zhang, S.},
abstractNote = {We present an improved search for axionlike polarization oscillations in the cosmic microwave background (CMB) with observations from the Keck Array. An all-sky, temporally sinusoidal rotation of CMB polarization, equivalent to a time-variable cosmic birefringence, is an observable manifestation of a local axion field and potentially allows a CMB polarimeter to detect axionlike dark matter directly. We describe improvements to the method presented in previous work, and we demonstrate the updated method with an expanded dataset consisting of the 2012–2015 observing seasons. We set limits on the axion-photon coupling constant for mass m in the range 10-23–10-18 eV, which corresponds to oscillation periods on the order of hours to years. Our results are consistent with the background model. For periods between 1 and 30 d (1.6×10-21≤m≤4.8×10-20 eV), the 95%-confidence upper limits on rotation amplitude are approximately constant with a median of 0.27°, which constrains the axion-photon coupling constant to gφγ<(4.5×10-12 GeV-1)m/(10-21 eV), if axionlike particles constitute all of the dark matter. More than half of the collected BICEP dataset has yet to be analyzed, and several current and future CMB polarimetry experiments can apply the methods presented here to achieve comparable or superior constraints. In the coming years, oscillation measurements can achieve the sensitivity to rule out unexplored regions of the axion parameter space.},
doi = {10.1103/physrevd.105.022006},
journal = {Physical Review. D.},
number = 2,
volume = 105,
place = {United States},
year = {Fri Jan 28 00:00:00 EST 2022},
month = {Fri Jan 28 00:00:00 EST 2022}
}

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