A demonstration of improved constraints on primordial gravitational waves with delensing

• Published in: Physical Review D
• Main Authors: Ade, P.A.R., Ahmed, Z., Amiri, M., Anderson, A.J., Austermann, J.E., Avva, J.S., Barkats, D., Basu Thakur, R., Beall, J.A., Bender, A.N., Benson, B.A., Bianchini, F., Bischoff, C.A., Bleem, L.E., Bock, J.J., Boenish, H., Bullock, E., Buza, V., Carlstrom, J.E., Chang, C.L., Cheshire, J.R., Chiang, H.C., Chou, T-L., Citron, R., Connors, J., Corbett Moran, C., Cornelison, J., Crawford, T.M., Crites, A.T., Crumrine, M., Cukierman, A., de Haan, T., Dierickx, M., Dobbs, M.A., Duband, L., Everett, W., Fatigoni, S., Filippini, J.P., Fliescher, S., Gallicchio, J., George, E.M., Germaine, T.St., Goeckner-Wald, N., Goldfinger, D.C., Grayson, J., Gupta, N., Hall, G., Halpern, M., Halverson, N.W., Harrison, S., Henderson, S., Henning, J.W., Hildebrandt, S.R., Hilton, G.C., Holder, G.P., Holzapfel, W.L., Hrubes, J.D., Huang, N., Hubmayr, J., Hui, H., Irwin, K.D., Kang, J., Karkare, K.S., Karpel, E., Kefeli, S., Kernasovskiy, S.A., Knox, L., Kovac, J.M., Kuo, C.L., Lau, K., Lee, A.T., Leitch, E.M., Li, D., Lowitz, A., Manzotti, A., Mcmahon, J.J., Megerian, K.G., Meyer, S.S., Millea, M., Mocanu, L.M., Moncelsi, L., Montgomery, J., Nadolski, A., Namikawa, T., Natoli, T., Netterfield, C.B., Nguyen, H.T., Nibarger, J.P., Noble, G., Novosad, V., O'Brient, R., Ogburn, R.W., Omori, Y., Padin, S., Palladino, S., Patil, S., Prouve, T., Pryke, C., Racine, B., Reichardt, C.L., Reintsema, C.D., Richter, S., Ruhl, J.E., Saliwanchik, B.R., Schaffer, K.K., Schillaci, A., Schmitt, B.L., Schwarz, R., Sheehy, C.D., Sievers, C., Smecher, G., Soliman, A., Stark, A.A., Steinbach, B., Sudiwala, R.V., Teply, G.P., Thompson, K.L., Tolan, J.E., Tucker, C., Turner, A.D., Umiltà, C., Veach, T., Vieira, J.D., Vieregg, A.G., Wandui, A., Wang, Gang, Weber, A.C., Whitehorn, N., Wiebe, D.V., Willmert, J., Wong, C.L., Wu, W.L.K., Yang, H., Yefremenko, V., Yoon, K.W., Young, E., Yu, C., Zeng, L., Zhang, C.
• Other Authors: Cardiff University, SLAC National Accelerator Laboratory (SLAC), Stanford University, University of British Columbia (UBC), Fermi National Accelerator Laboratory (Fermilab), National Institute of Standards and Technology Boulder (NIST), University of Colorado Boulder, University of California Berkeley (UC Berkeley), University of California (UC), Harvard-Smithsonian Center for Astrophysics (CfA), Harvard University-Smithsonian Institution, California Institute of Technology (CALTECH), Argonne National Laboratory Lemont (ANL), Kavli Institute for Cosmological Physics Chicago (KICP), University of Chicago, University of Melbourne, University of Cincinnati (UC), Jet Propulsion Laboratory (JPL), NASA-California Institute of Technology (CALTECH), Harvard University, Département des Systèmes Basses Températures (DSBT ), Institut de Recherche Interdisciplinaire de Grenoble (IRIG), Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Direction de Recherche Fondamentale (CEA) (DRF (CEA)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Grenoble Alpes (UGA), Institut d'Astrophysique de Paris (IAP), Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), SPTpol, BICEP/Keck
• Format: Article in Journal/Newspaper
• Language: English
• Published: HAL CCSD 2021
• Subjects: gravitation: lens; gravitational radiation: primordial; satellite: Planck; cosmic background radiation; BICEP; polarization; B-mode; infrared; background; data analysis method; statistical analysis; cosmic background radiation: polarization; numerical calculations; Experiments in gravity; cosmology; cosmic rays; [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]; South pole
• Online Access: https://hal.science/hal-03047658; https://hal.science/hal-03047658/document; https://hal.science/hal-03047658/file/AdeEtAl21.pdf; https://doi.org/10.1103/PhysRevD.103.022004

International audience We present a constraint on the tensor-to-scalar ratio, r, derived from measurements of cosmic microwave background (CMB) polarization B-modes with “delensing,” whereby the uncertainty on r contributed by the sample variance of the gravitational lensing B-modes is reduced by cross-correlating against a lensing B-mode template. This template is constructed by combining an estimate of the polarized CMB with a tracer of the projected large-scale structure. The large-scale-structure tracer used is a map of the cosmic infrared background derived from Planck satellite data, while the polarized CMB map comes from a combination of South Pole Telescope, bicep/Keck, and Planck data. We expand the bicep/Keck likelihood analysis framework to accept a lensing template and apply it to the bicep/Keck dataset collected through 2014 using the same parametric foreground modeling as in the previous analysis. From simulations, we find that the uncertainty on r is reduced by ∼10%, from σ(r)=0.024 to 0.022, which can be compared with a ∼26% reduction obtained when using a perfect lensing template or if there were zero lensing B-modes. Applying the technique to the real data, the constraint on r is improved from r0.05<0.090 to r0.05<0.082 (95% C.L.). This is the first demonstration of improvement in an r constraint through delensing.