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Title: Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season

Abstract

Here, we present results from an analysis of all data taken by the BICEP2, Keck Array, and BICEP3 CMB polarization experiments up to and including the 2018 observing season. We add additional Keck Array observations at 220 GHz and BICEP3 observations at 95 GHz to the previous 95/150/220 GHz dataset. The Q/U maps now reach depths of 2.8, 2.8, and 8.8 μKCMB arcmin at 95,150, and 220 GHz, respectively, over an effective area of ≈ 600 square degrees at 95 GHz and ≈ 400 square degrees at 150 and 220 GHz. The 220 GHz maps now achieve a signal-to-noise ratio on polarized dust emission exceeding that of Planck at 353 GHz. We take auto- and cross-spectra between these maps and publicly available WMAP and Planck maps at frequencies from 23 to 353 GHz and evaluate the joint likelihood of the spectra versus a multicomponent model of lensed ΛCDM + r + dust + synchrotron + noise . The foreground model has seven parameters, and no longer requires a prior on the frequency spectral index of the dust emission taken from measurements on other regions of the sky. This model is an adequate description of the data at the current noisemore » levels. The likelihood analysis yields the constraint r 0.05 < 0.036 at 95% confidence. Running maximum likelihood search on simulations we obtain unbiased results and find that σ(r) = 0.009 . These are the strongest constraints to date on primordial gravitational waves.« less

Authors:
 [1]; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; more »; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; ; « less
  1. Cardiff Univ., Wales (United Kingdom); BICEP/Keck Collaboration. et al.
Publication Date:
Research Org.:
SLAC National Accelerator Lab., Menlo Park, CA (United States); Brookhaven National Lab. (BNL), Upton, NY (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF); National Aeronautical and Space Administration (NASA)
Contributing Org.:
BICEP/Keck Collaboration
OSTI Identifier:
1870843
Grant/Contract Number:  
AC02-76SF00515; 0742818; 0742592; 1044978; 1110087; 1145172; 1145143; 1145248; 1639040; 1638957; 1638978; 1638970; 06-ARPA206-0040; 10-SAT10-0017; 12- SAT12-0031; 14-SAT14-0009; 16-SAT-16- 0002
Resource Type:
Accepted Manuscript
Journal Name:
Physical Review Letters
Additional Journal Information:
Journal Volume: 127; Journal Issue: 15; Journal ID: ISSN 0031-9007
Publisher:
American Physical Society (APS)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; cosmic microwave background; cosmological parameters; inflation

Citation Formats

Ade, P.  A. R., Ahmed, Z., Amiri, M., Barkats, D., Thakur, R. Basu, 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. Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season. United States: N. p., 2021. Web. doi:10.1103/physrevlett.127.151301.
Ade, P.  A. R., Ahmed, Z., Amiri, M., Barkats, D., Thakur, R. Basu, 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. Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season. United States. https://doi.org/10.1103/physrevlett.127.151301
Ade, P.  A. R., Ahmed, Z., Amiri, M., Barkats, D., Thakur, R. Basu, 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. Mon . "Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season". United States. https://doi.org/10.1103/physrevlett.127.151301. https://www.osti.gov/servlets/purl/1870843.
@article{osti_1870843,
title = {Improved Constraints on Primordial Gravitational Waves using Planck, WMAP, and BICEP/Keck Observations through the 2018 Observing Season},
author = {Ade, P.  A. R. and Ahmed, Z. and Amiri, M. and Barkats, D. and Thakur, R. Basu 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 = {Here, we present results from an analysis of all data taken by the BICEP2, Keck Array, and BICEP3 CMB polarization experiments up to and including the 2018 observing season. We add additional Keck Array observations at 220 GHz and BICEP3 observations at 95 GHz to the previous 95/150/220 GHz dataset. The Q/U maps now reach depths of 2.8, 2.8, and 8.8 μKCMB arcmin at 95,150, and 220 GHz, respectively, over an effective area of ≈ 600 square degrees at 95 GHz and ≈ 400 square degrees at 150 and 220 GHz. The 220 GHz maps now achieve a signal-to-noise ratio on polarized dust emission exceeding that of Planck at 353 GHz. We take auto- and cross-spectra between these maps and publicly available WMAP and Planck maps at frequencies from 23 to 353 GHz and evaluate the joint likelihood of the spectra versus a multicomponent model of lensed ΛCDM + r + dust + synchrotron + noise . The foreground model has seven parameters, and no longer requires a prior on the frequency spectral index of the dust emission taken from measurements on other regions of the sky. This model is an adequate description of the data at the current noise levels. The likelihood analysis yields the constraint r 0.05 < 0.036 at 95% confidence. Running maximum likelihood search on simulations we obtain unbiased results and find that σ(r) = 0.009 . These are the strongest constraints to date on primordial gravitational waves.},
doi = {10.1103/physrevlett.127.151301},
journal = {Physical Review Letters},
number = 15,
volume = 127,
place = {United States},
year = {Mon Oct 04 00:00:00 EDT 2021},
month = {Mon Oct 04 00:00:00 EDT 2021}
}

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