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CMBPol Mission Concept Study: Probing Inflation with CMB Polarization
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 w...
Autores principales: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Lenguaje: | eng |
Publicado: |
2008
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1063/1.3160885 http://cds.cern.ch/record/1141848 |
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author | Baumann, Daniel Jackson, Mark G. Adshead, Peter Amblard, Alexandre Ashoorioon, Amjad Bartolo, Nicola Bean, Rachel Beltran, Maria de Bernardis, Francesco Bird, Simeon Chen, Xingang Chung, Daniel Jun Hun Colombo, Loris Cooray, Asantha R. Creminelli, Paolo Dodelson, Scott Dunkley, Joanna Dvorkin, Cora Easther, Richard Finelli, Fabio Flauger, Raphael Hertzberg, Mark P. Jones-Smith, Katherine Kachru, Shamit Kadota, Kenji Khoury, Justin Kinney, William H. Komatsu, Eiichiro Krauss, Lawrence M. Lesgourgues, Julien Liddle, Andrew R. Liguori, Michele Lim, Eugene A. Linde, Andrei D. Matarrese, Sabino Mathur, Harsh McAllister, Liam Melchiorri, Alessandro Nicolis, Alberto Pagano, Luca Peiris, Hiranya V. Peloso, Marco Pogosian, Levon Pierpaoli, Elena Riotto, Antonio Seljak, Uros Senatore, Leonardo Shandera, Sarah E. Silverstein, Eva Smith, Tristan Vaudrevange, Pascal M. Verde, Licia Wandelt, Ben Wands, David Watson, Scott Wyman, Mark Yadav, Amit Valkenburg, Wessel Zaldarriaga, Matias |
author_facet | Baumann, Daniel Jackson, Mark G. Adshead, Peter Amblard, Alexandre Ashoorioon, Amjad Bartolo, Nicola Bean, Rachel Beltran, Maria de Bernardis, Francesco Bird, Simeon Chen, Xingang Chung, Daniel Jun Hun Colombo, Loris Cooray, Asantha R. Creminelli, Paolo Dodelson, Scott Dunkley, Joanna Dvorkin, Cora Easther, Richard Finelli, Fabio Flauger, Raphael Hertzberg, Mark P. Jones-Smith, Katherine Kachru, Shamit Kadota, Kenji Khoury, Justin Kinney, William H. Komatsu, Eiichiro Krauss, Lawrence M. Lesgourgues, Julien Liddle, Andrew R. Liguori, Michele Lim, Eugene A. Linde, Andrei D. Matarrese, Sabino Mathur, Harsh McAllister, Liam Melchiorri, Alessandro Nicolis, Alberto Pagano, Luca Peiris, Hiranya V. Peloso, Marco Pogosian, Levon Pierpaoli, Elena Riotto, Antonio Seljak, Uros Senatore, Leonardo Shandera, Sarah E. Silverstein, Eva Smith, Tristan Vaudrevange, Pascal M. Verde, Licia Wandelt, Ben Wands, David Watson, Scott Wyman, Mark Yadav, Amit Valkenburg, Wessel Zaldarriaga, Matias |
author_sort | Baumann, Daniel |
collection | CERN |
description | 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. |
id | cern-1141848 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2008 |
record_format | invenio |
spelling | cern-11418482023-08-02T03:09:36Zdoi:10.1063/1.3160885http://cds.cern.ch/record/1141848engBaumann, DanielJackson, Mark G.Adshead, PeterAmblard, AlexandreAshoorioon, AmjadBartolo, NicolaBean, RachelBeltran, Mariade Bernardis, FrancescoBird, SimeonChen, XingangChung, Daniel Jun HunColombo, LorisCooray, Asantha R.Creminelli, PaoloDodelson, ScottDunkley, JoannaDvorkin, CoraEasther, RichardFinelli, FabioFlauger, RaphaelHertzberg, Mark P.Jones-Smith, KatherineKachru, ShamitKadota, KenjiKhoury, JustinKinney, William H.Komatsu, EiichiroKrauss, Lawrence M.Lesgourgues, JulienLiddle, Andrew R.Liguori, MicheleLim, Eugene A.Linde, Andrei D.Matarrese, SabinoMathur, HarshMcAllister, LiamMelchiorri, AlessandroNicolis, AlbertoPagano, LucaPeiris, Hiranya V.Peloso, MarcoPogosian, LevonPierpaoli, ElenaRiotto, AntonioSeljak, UrosSenatore, LeonardoShandera, Sarah E.Silverstein, EvaSmith, TristanVaudrevange, Pascal M.Verde, LiciaWandelt, BenWands, DavidWatson, ScottWyman, MarkYadav, AmitValkenburg, WesselZaldarriaga, MatiasCMBPol Mission Concept Study: Probing Inflation with CMB PolarizationAstrophysics and AstronomyWe 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.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.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.arXiv:0811.3919FERMILAB-PUB-08-601-ACERN-PH-TH-2008-230oai:cds.cern.ch:11418482008-11-25 |
spellingShingle | Astrophysics and Astronomy Baumann, Daniel Jackson, Mark G. Adshead, Peter Amblard, Alexandre Ashoorioon, Amjad Bartolo, Nicola Bean, Rachel Beltran, Maria de Bernardis, Francesco Bird, Simeon Chen, Xingang Chung, Daniel Jun Hun Colombo, Loris Cooray, Asantha R. Creminelli, Paolo Dodelson, Scott Dunkley, Joanna Dvorkin, Cora Easther, Richard Finelli, Fabio Flauger, Raphael Hertzberg, Mark P. Jones-Smith, Katherine Kachru, Shamit Kadota, Kenji Khoury, Justin Kinney, William H. Komatsu, Eiichiro Krauss, Lawrence M. Lesgourgues, Julien Liddle, Andrew R. Liguori, Michele Lim, Eugene A. Linde, Andrei D. Matarrese, Sabino Mathur, Harsh McAllister, Liam Melchiorri, Alessandro Nicolis, Alberto Pagano, Luca Peiris, Hiranya V. Peloso, Marco Pogosian, Levon Pierpaoli, Elena Riotto, Antonio Seljak, Uros Senatore, Leonardo Shandera, Sarah E. Silverstein, Eva Smith, Tristan Vaudrevange, Pascal M. Verde, Licia Wandelt, Ben Wands, David Watson, Scott Wyman, Mark Yadav, Amit Valkenburg, Wessel Zaldarriaga, Matias CMBPol Mission Concept Study: Probing Inflation with CMB Polarization |
title | CMBPol Mission Concept Study: Probing Inflation with CMB Polarization |
title_full | CMBPol Mission Concept Study: Probing Inflation with CMB Polarization |
title_fullStr | CMBPol Mission Concept Study: Probing Inflation with CMB Polarization |
title_full_unstemmed | CMBPol Mission Concept Study: Probing Inflation with CMB Polarization |
title_short | CMBPol Mission Concept Study: Probing Inflation with CMB Polarization |
title_sort | cmbpol mission concept study: probing inflation with cmb polarization |
topic | Astrophysics and Astronomy |
url | https://dx.doi.org/10.1063/1.3160885 http://cds.cern.ch/record/1141848 |
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