Probing inflation with CMB polarization

Daniel Baumann; Mark G. Jackson; Peter Adshead; Alexandre Amblard; Amjad Ashoorioon; Nicola Bartolo; Rachel Bean; Maria Beltrán; Francesco De Bernardis; Simeon Bird; Xingang Chen; Daniel J.H. Chung; Loris Colombo; Asantha Cooray; Paolo Creminelli; Scott Dodelson; Joanna Dunkley; Cora Dvorkin; Richard Easther; Fabio Finelli; Raphael Flauger; Mark P. Hertzberg; Katherine Jones-Smith; Shamit Kachru; Kenji Kadota; Justin Khoury; William H. Kinney; Eiichiro Komatsu; Lawrence M. Krauss; Julien Lesgourgues; Andrew Liddle; Michele Liguori; Eugene Lim; Andrei Linde; Sabino Matarrese; Harsh Mathur; Liam McAllister; Alessandro Melchiorri; Alberto Nicolis; Luca Pagano; Hiranya V. Peiris; Marco Peloso; Levon Pogosian; Elena Pierpaoli; Antonio Riotto; Uroš Seljak; Leonardo Senatore; Sarah Shandera; Eva Silverstein; Tristan Smith; Pascal Vaudrevange; Licia Verde; Ben Wandelt; David Wands; Scott Watson; Mark Wyman; Amit Yadav; Wessel Valkenburg; Matias Zaldarriaga

doi:10.1063/1.3160885

Probing inflation with CMB polarization

Daniel Baumann
, Mark G. Jackson
, Peter Adshead
, Alexandre Amblard
, Amjad Ashoorioon
, Nicola Bartolo
, Rachel Bean
, Maria Beltrán
, Francesco De Bernardis
, Simeon Bird
, Xingang Chen
, Daniel J.H. Chung
, Loris Colombo
, Asantha Cooray
, Paolo Creminelli
, Scott Dodelson
, Joanna Dunkley
, Cora Dvorkin
, Richard Easther
, Fabio Finelli

Raphael Flauger, Mark P. Hertzberg, Katherine Jones-Smith, Shamit Kachru, Kenji Kadota, Justin Khoury, William H. Kinney, Eiichiro Komatsu, Lawrence M. Krauss, Julien Lesgourgues, Andrew Liddle, Michele Liguori, Eugene Lim, Andrei Linde, Sabino Matarrese, Harsh Mathur, Liam McAllister, Alessandro Melchiorri, Alberto Nicolis, Luca Pagano, Hiranya V. Peiris, Marco Peloso, Levon Pogosian, Elena Pierpaoli, Antonio Riotto, Uroš Seljak, Leonardo Senatore, Sarah Shandera, Eva Silverstein, Tristan Smith, Pascal Vaudrevange, Licia Verde, Ben Wandelt, David Wands, Scott Watson, Mark Wyman, Amit Yadav, Wessel Valkenburg, Matias Zaldarriaga

Physics

Harvard University
Princeton University
Fermi National Accelerator Laboratory
Leiden University
Yale University
University of California at Irvine
University of Michigan, Ann Arbor
University of Padua
Cornell University
The University of Chicago
University of Rome La Sapienza
University of Cambridge
Massachusetts Institute of Technology
University of Wisconsin-Madison
University of Southern California
Abdus Salam International Centre for Theoretical Physics
Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
Osservatorio Astronomico di Bologna
National Institute for Nuclear Physics
University of Texas at Austin
Case Western Reserve University
SLAC National Accelerator Laboratory
University of Minnesota Twin Cities
Perimeter Institute for Theoretical Physics
Arizona State University
CERN
Swiss Federal Institute of Technology Lausanne
Université Savoie Mont Blanc
University of Sussex
Columbia University
Simon Fraser University
University of California at Berkeley
University of Zurich
California Institute of Technology
University of Toronto
Campus UAB
University of Illinois at Urbana-Champaign
University of Portsmouth

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

302 Scopus citations

Abstract

We summarize the utility of precise cosmic microwave background (CMB) polarization measurements as probes of the physics of inflation. We focus on the prospects for using CMB measurements to differentiate various inflationary mechanisms. In particular, a detection of primordial B-mode polarization would demonstrate that inflation occurred at a very high energy scale, and that the inflaton traversed a super-Planckian distance in field space. We explain how such a detection or constraint would illuminate aspects of physics at the Planck scale. Moreover, CMB measurements can constrain the scale-dependence and non-Gaussianity of the primordial fluctuations and limit the possibility of a significant isocurvature contribution. Each such limit provides crucial information on the underlying inflationary dynamics. Finally, we quantify these considerations by presenting forecasts for the sensitivities of a future satellite experiment to the inflationary parameters.

Original language	English
Title of host publication	CMB Polarization Workshop
Subtitle of host publication	Theory and Foregrounds - CMBPol Mission Concept Study
Publisher	American Institute of Physics Inc.
Pages	10-120
Number of pages	111
ISBN (Print)	9780735406780
DOIs	https://doi.org/10.1063/1.3160885
State	Published - 2009
Event	CMB Polarization Workshop: Theory And Foregrounds - Batavia, IL, United States Duration: Jun 23 2008 → Jun 26 2008

Publication series

Name	AIP Conference Proceedings
Volume	1141
ISSN (Print)	0094-243X
ISSN (Electronic)	1551-7616

Conference

Conference	CMB Polarization Workshop: Theory And Foregrounds
Country/Territory	United States
City	Batavia, IL
Period	06/23/08 → 06/26/08

Access to Document

10.1063/1.3160885

Cite this

Baumann, D., Jackson, M. G., Adshead, P., Amblard, A., Ashoorioon, A., Bartolo, N., Bean, R., Beltrán, M., Bernardis, F. D., Bird, S., Chen, X., Chung, D. J. H., Colombo, L., Cooray, A., Creminelli, P., Dodelson, S., Dunkley, J., Dvorkin, C., Easther, R., ... Zaldarriaga, M. (2009). Probing inflation with CMB polarization. In CMB Polarization Workshop: Theory and Foregrounds - CMBPol Mission Concept Study (pp. 10-120). (AIP Conference Proceedings; Vol. 1141). American Institute of Physics Inc.. https://doi.org/10.1063/1.3160885

@inproceedings{8e6e001490174356844b593a9cdd0098,

title = "Probing inflation with CMB polarization",

abstract = "We summarize the utility of precise cosmic microwave background (CMB) polarization measurements as probes of the physics of inflation. We focus on the prospects for using CMB measurements to differentiate various inflationary mechanisms. In particular, a detection of primordial B-mode polarization would demonstrate that inflation occurred at a very high energy scale, and that the inflaton traversed a super-Planckian distance in field space. We explain how such a detection or constraint would illuminate aspects of physics at the Planck scale. Moreover, CMB measurements can constrain the scale-dependence and non-Gaussianity of the primordial fluctuations and limit the possibility of a significant isocurvature contribution. Each such limit provides crucial information on the underlying inflationary dynamics. Finally, we quantify these considerations by presenting forecasts for the sensitivities of a future satellite experiment to the inflationary parameters.",

author = "Daniel Baumann and Jackson, \{Mark G.\} and Peter Adshead and Alexandre Amblard and Amjad Ashoorioon and Nicola Bartolo and Rachel Bean and Maria Beltr{\'a}n and Bernardis, \{Francesco De\} and Simeon Bird and Xingang Chen and Chung, \{Daniel J.H.\} and Loris Colombo and Asantha Cooray and Paolo Creminelli and Scott Dodelson and Joanna Dunkley and Cora Dvorkin and Richard Easther and Fabio Finelli and Raphael Flauger and Hertzberg, \{Mark P.\} and Katherine Jones-Smith and Shamit Kachru and Kenji Kadota and Justin Khoury and Kinney, \{William H.\} and Eiichiro Komatsu and Krauss, \{Lawrence M.\} and Julien Lesgourgues and Andrew Liddle and Michele Liguori and Eugene Lim and Andrei Linde and Sabino Matarrese and Harsh Mathur and Liam McAllister and Alessandro Melchiorri and Alberto Nicolis and Luca Pagano and Peiris, \{Hiranya V.\} and Marco Peloso and Levon Pogosian and Elena Pierpaoli and Antonio Riotto and Uro{\v s} Seljak and Leonardo Senatore and Sarah Shandera and Eva Silverstein and Tristan Smith and Pascal Vaudrevange and Licia Verde and Ben Wandelt and David Wands and Scott Watson and Mark Wyman and Amit Yadav and Wessel Valkenburg and Matias Zaldarriaga",

year = "2009",

doi = "10.1063/1.3160885",

language = "English",

isbn = "9780735406780",

series = "AIP Conference Proceedings",

publisher = "American Institute of Physics Inc.",

pages = "10--120",

booktitle = "CMB Polarization Workshop",

note = "CMB Polarization Workshop: Theory And Foregrounds ; Conference date: 23-06-2008 Through 26-06-2008",

}

Baumann, D, Jackson, MG, Adshead, P, Amblard, A, Ashoorioon, A, Bartolo, N, Bean, R, Beltrán, M, Bernardis, FD, Bird, S, Chen, X, Chung, DJH, Colombo, L, Cooray, A, Creminelli, P, Dodelson, S, Dunkley, J, Dvorkin, C, Easther, R, Finelli, F, Flauger, R, Hertzberg, MP, Jones-Smith, K, Kachru, S, Kadota, K, Khoury, J, Kinney, WH, Komatsu, E, Krauss, LM, Lesgourgues, J, Liddle, A, Liguori, M, Lim, E, Linde, A, Matarrese, S, Mathur, H, McAllister, L, Melchiorri, A, Nicolis, A, Pagano, L, Peiris, HV, Peloso, M, Pogosian, L, Pierpaoli, E, Riotto, A, Seljak, U, Senatore, L, Shandera, S, Silverstein, E, Smith, T, Vaudrevange, P, Verde, L, Wandelt, B, Wands, D, Watson, S, Wyman, M, Yadav, A, Valkenburg, W & Zaldarriaga, M 2009, Probing inflation with CMB polarization. in CMB Polarization Workshop: Theory and Foregrounds - CMBPol Mission Concept Study. AIP Conference Proceedings, vol. 1141, American Institute of Physics Inc., pp. 10-120, CMB Polarization Workshop: Theory And Foregrounds, Batavia, IL, United States, 06/23/08. https://doi.org/10.1063/1.3160885

Probing inflation with CMB polarization. / Baumann, Daniel; Jackson, Mark G.; Adshead, Peter et al.
CMB Polarization Workshop: Theory and Foregrounds - CMBPol Mission Concept Study. American Institute of Physics Inc., 2009. p. 10-120 (AIP Conference Proceedings; Vol. 1141).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › peer-review

TY - GEN

T1 - Probing inflation with CMB polarization

AU - Baumann, Daniel

AU - Jackson, Mark G.

AU - Adshead, Peter

AU - Amblard, Alexandre

AU - Ashoorioon, Amjad

AU - Bartolo, Nicola

AU - Bean, Rachel

AU - Beltrán, Maria

AU - Bernardis, Francesco De

AU - Bird, Simeon

AU - Chen, Xingang

AU - Chung, Daniel J.H.

AU - Colombo, Loris

AU - Cooray, Asantha

AU - Creminelli, Paolo

AU - Dodelson, Scott

AU - Dunkley, Joanna

AU - Dvorkin, Cora

AU - Easther, Richard

AU - Finelli, Fabio

AU - Flauger, Raphael

AU - Hertzberg, Mark P.

AU - Jones-Smith, Katherine

AU - Kachru, Shamit

AU - Kadota, Kenji

AU - Khoury, Justin

AU - Kinney, William H.

AU - Komatsu, Eiichiro

AU - Krauss, Lawrence M.

AU - Lesgourgues, Julien

AU - Liddle, Andrew

AU - Liguori, Michele

AU - Lim, Eugene

AU - Linde, Andrei

AU - Matarrese, Sabino

AU - Mathur, Harsh

AU - McAllister, Liam

AU - Melchiorri, Alessandro

AU - Nicolis, Alberto

AU - Pagano, Luca

AU - Peiris, Hiranya V.

AU - Peloso, Marco

AU - Pogosian, Levon

AU - Pierpaoli, Elena

AU - Riotto, Antonio

AU - Seljak, Uroš

AU - Senatore, Leonardo

AU - Shandera, Sarah

AU - Silverstein, Eva

AU - Smith, Tristan

AU - Vaudrevange, Pascal

AU - Verde, Licia

AU - Wandelt, Ben

AU - Wands, David

AU - Watson, Scott

AU - Wyman, Mark

AU - Yadav, Amit

AU - Valkenburg, Wessel

AU - Zaldarriaga, Matias

PY - 2009

Y1 - 2009

N2 - We summarize the utility of precise cosmic microwave background (CMB) polarization measurements as probes of the physics of inflation. We focus on the prospects for using CMB measurements to differentiate various inflationary mechanisms. In particular, a detection of primordial B-mode polarization would demonstrate that inflation occurred at a very high energy scale, and that the inflaton traversed a super-Planckian distance in field space. We explain how such a detection or constraint would illuminate aspects of physics at the Planck scale. Moreover, CMB measurements can constrain the scale-dependence and non-Gaussianity of the primordial fluctuations and limit the possibility of a significant isocurvature contribution. Each such limit provides crucial information on the underlying inflationary dynamics. Finally, we quantify these considerations by presenting forecasts for the sensitivities of a future satellite experiment to the inflationary parameters.

AB - We summarize the utility of precise cosmic microwave background (CMB) polarization measurements as probes of the physics of inflation. We focus on the prospects for using CMB measurements to differentiate various inflationary mechanisms. In particular, a detection of primordial B-mode polarization would demonstrate that inflation occurred at a very high energy scale, and that the inflaton traversed a super-Planckian distance in field space. We explain how such a detection or constraint would illuminate aspects of physics at the Planck scale. Moreover, CMB measurements can constrain the scale-dependence and non-Gaussianity of the primordial fluctuations and limit the possibility of a significant isocurvature contribution. Each such limit provides crucial information on the underlying inflationary dynamics. Finally, we quantify these considerations by presenting forecasts for the sensitivities of a future satellite experiment to the inflationary parameters.

UR - https://www.scopus.com/pages/publications/69949123764

U2 - 10.1063/1.3160885

DO - 10.1063/1.3160885

M3 - Conference contribution

AN - SCOPUS:69949123764

SN - 9780735406780

T3 - AIP Conference Proceedings

SP - 10

EP - 120

BT - CMB Polarization Workshop

PB - American Institute of Physics Inc.

T2 - CMB Polarization Workshop: Theory And Foregrounds

Y2 - 23 June 2008 through 26 June 2008

ER -

Probing inflation with CMB polarization

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