CMB-S4 Science Book, First Edition

Kevork N. Abazajian, Peter Adshead, Zeeshan Ahmed, Steven W. Allen, David Alonso, Kam S. Arnold, Carlo Baccigalupi, James G. Bartlett, Nicholas Battaglia, Bradford A. Benson, Colin A. Bischoff, Julian Borrill, Victor Buza, Erminia Calabrese, Robert Caldwell, John E. Carlstrom, Clarence L. Chang, Thomas M. Crawford, Francis-Yan Cyr-Racine, Francesco De BernardisTijmen de Haan, Sperello di Serego Alighieri, Joanna Dunkley, Cora Dvorkin, Josquin Errard, Giulio Fabbian, Stephen Feeney, Simone Ferraro, Jeffrey P. Filippini, Raphael Flauger, George M. Fuller, Vera Gluscevic, Daniel Green, Daniel Grin, Evan Grohs, Jason W. Henning, J. Colin Hill, Renee Hlozek, Gilbert Holder, William Holzapfel, Wayne Hu, Kevin M. Huffenberger, Reijo Keskitalo, Lloyd Knox, Arthur Kosowsky, John Kovac, Ely D. Kovetz, Chao-Lin Kuo, Akito Kusaka, Maude Le Jeune, Adrian T. Lee, Marc Lilley, Marilena Loverde, Mathew S. Madhavacheril, Adam Mantz, David J. E. Marsh, Jeffrey McMahon, Pieter Daniel Meerburg, Joel Meyers, Amber D. Miller, Julian B. Munoz, Ho Nam Nguyen, Michael D. Niemack, Marco Peloso, Julien Peloton, Levon Pogosian, Clement Pryke, Marco Raveri, Christian L. Reichardt, Graca Rocha, Aditya Rotti, Emmanuel Schaan, Marcel M. Schmittfull, Douglas Scott, Neelima Sehgal, Sarah Shandera, Blake D. Sherwin, Tristan L. Smith, Lorenzo Sorbo, Glenn D. Starkman, Kyle T. Story, Alexander van Engelen, Joaquin D. Vieira, Scott Watson, Nathan Whitehorn, W. L. Kimmy Wu

Research output: Book/ReportBookAcademic

Abstract

This book lays out the scientific goals to be addressed by the next-generation ground-based cosmic microwave background experiment, CMB-S4, envisioned to consist of dedicated telescopes at the South Pole, the high Chilean Atacama plateau and possibly a northern hemisphere site, all equipped with new superconducting cameras. CMB-S4 will dramatically advance cosmological studies by crossing critical thresholds in the search for the B-mode polarization signature of primordial gravitational waves, in the determination of the number and masses of the neutrinos, in the search for evidence of new light relics, in constraining the nature of dark energy, and in testing general relativity on large scales.
Original languageEnglish
Publication statusPublished - 10-Oct-2016
Externally publishedYes

Publication series

NameFermilab

Keywords

  • astro-ph.CO
  • gr-qc
  • hep-ph
  • hep-th

Cite this