CMBPol Mission Concept Study. Stephan Meyer Unversity of Chicago July 28, 2008
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1 CMBPol Mission Concept Study Stephan Meyer Unversity of Chicago July 28, 2008
2 this study? o enhance the priority of inflation science within the funding agencies. There is an opportunity to do this because the 2010 NRC Decadal Surve of Astrophysics will begin its wor in the Fall 2008 and accept input from communities through early 2009.
3 e Astrophysics Division of the ssion Concept Studie cience Mission Directorate olicits concept studies for trategic space flight science issions that may be carried out n the next decade or for which echnology development funding is ought in the next decade. e goal of the mission concept tudies is to develop high-quality cientific, technical, and cost nformation to be used for future
4 Decadal Surveys 1990 Bahcall 2000 McKee-Tayl he surveys take an overview of the state of astrophysics and make a prioritized list of recommendations for the upcoming decade.
5
6 0
7 flation science can be on a milar list in the 2010 cadal Report if: the science case is compelling a coherent, realistic plan exists the CMB community speaks in unison.
8 stablish the fundamental importance nflation science. smology trophysics rticle Physics ocument the experimental feasibilit f significantly constraining nflationary models. rm theoretical predictions of observables e state of technology (two instrument udies) turity of experimental techniques
9 Get input from the broad scientific community. What we agree on. What we do not agree on - Document the various positions - Identify the research and investigations needed to come to an optimum (acceptable) resoluti Entire process is open to input from a There will be a period of Request fo
10 . Develop a path to getting the most science out of the information available in the CMB polarization measurement in the next decade.. Generate a report for the NRC Decada Survey on Astrophysics. Influence the text of the survey Establish a high priority for CMB inflation science
11 be? The plan has still to evolve over the next four months while the There is a programmatic hold on a start of a medium-scale space missi because of the BEPAC findings. Much will be learned in the next 5 7 years from Planck and suborbital experiments and the research they inspire. study is being developed. the most general level:
12 ingoing thoughts on the best plan sent to the decadal panel is: ve a comprehensive overview of the portance of inflationary science r cosmology, astrophysics and ysics. tline the galactic and extralactic astrophysics which will com om a CMB polarization mission. ke an overview of the state of rrent technology and what we
13 Review the experimental techniques being developed. -Instrumentation -Systematics control -Analysis techniques -Foreground removal Make a strong case that this research will lead to a compelling space A central based question: mission proposal in mid decade. Does the plan promote a space mission now or one following 5 years of further results from
14 PI S. Meyer rkshop: heory, cillary cience egrounds Dodelson Workshop: Systematics Scan strategies Template missions G. Hinshaw/J. Ruhl Workshop: Technologies Detector systems Optical systems K. Irwin/S. Hanany ote s iled dy: groun s ooray Detailed Study: Amplifier Mission M.Seiffert/C.Lawrence Detailed Study: Detailed Detailed Lensing Study: Study: M. Scanning Foreground/ Zaldarriag Strategies feeds a K. Gorski L. Page/J. Dunkley Detailed Study: Bolometer Mission J. Bock Detaile Detailed Study: Study: Polariza Optics n A. Lee Systemat B. Keati
15 -Develop template missions with wel defined properties - Illustrate the capabilities we have today - Serve as baselines for compariso of scan strategy and foreground subtraction methods - Three templates will be used: EPIC, a concept proposed by Jami Bock An intermediate (~10 ) resolutio study A large (~4 ) resolution study
16 Input from the community * -Wide request for participation. -Three workshops open to everyone o four central topics: Theory, Foregrounds, Systematics and Technology. -Workshop summaries with an overvie which will be public and have an opportunity for input from people who are not part of the workshops. This is not just the US CMB community --
17 0 ple far e a t in pol dy Amjad Pablo Ashoorioon Fosalba Carlo Joseph Fowler Baccigalupi Aurelien Nicola Bartolo Fraisse Daniel Baumann Todd Gaier Rachel Bean Nick Gnedin Maria Beltran Krzysztof Gorski Dominic Benford Joshua Chuck BennettJ Gundersen ames Bock Shaul Hanany Julian Borrill Makoto Latham Boyle Hattori Emory Bunn Marijke Clarence Chang Haverkorn Xingang Chen Masashi Hazumi Daniel Chung Mark Sarah Church Hertzberg David Chuss James Asantha CoorayP Hinderks aolo Gary Creminelli Hinshaw Sudeep DasC Chris Hirata live Wayne Hu Dickinson Howard Hui Michael DiPirro Kent Irwin Matt Dobbs Mark Greg Dobler Jackson Scott onnie Jansson Dodelson Brad Olivier Dore Johnson Jessie Dotson Dean Thomas Downes Johnson William Duncan William Jones Joanna Dunkley Katherine Jones- Cora Dvorkin Smith Lesgourgues Andrew Liddle Adam Lidz Michele Liguori Eugene Lim Marilena Loverde Antonio Magalhaes Mario Magalhaes John Marriner Victoria Martin Sabino Matarrese Harsh Mathur Benjamin Mazin Liam McAllister Jeff McMahon Alessandro Melchiorri Gary Melnick Stephan Meyer Amber Miller Michael Mortonson Samuel Moseley Hogan Nguyen Alberto Nicolis Peng Oh Lyman Page Hiranya Peiris John Peoples Nicolas Phillips Peter Shirro Robert Silver Eva Silverstein Jean Slaugh Eric Smith Kendrick Smith Tristan Smith Glenn Starkm Albert Stebbi Jason Steffe Radek Stompo Osamu Tajima Peter Timbie Takayuki Tomaru Ray Tomlin Huan Tran Gregory Tucker Amol Upadhy John Vaillancourt Wessel Valken Pascal Vaudrevange Marcellla Venezi Licia VerdeJ oaquin Vieira Andre Waelke Ben Wandel David Wands Scott Watson William Wester Bruce Winste Edward Wollac Maik Wolleb Mark Wyman
18 Input from the community (continued -Workshop on theory and foregrounds last month -Organized by Scott Dodelson -Inflation -Reionization -Lensing -Foreground removal -Foreground science
19 Workshop on Systematics in 2 weeks. - Organized by Gary Hinshaw and John Ruhl - Experience from experiments with data - Plans for experiments in development and future - Experiment simulation and analysis -Workshop on Technology in late August - Organized by Shaul Hanany and Kent Irwin - Detection techniques - Optical coupling - Bands and filters - Readouts
20 Input from the community (continued -A group of participants will write summary of each of the topics in th workshops. -These will be summarized by the workshop organizers into a proceedings. -The workshop proceedings along with presentation slides will be on the CMBpol website. -They will provide the basis for the report to the decadal.
21 sections of the report based on the workshop proceedings. -Drafts of the report will be on the CMBPol website for comment. -In November, the report will be sent to reviewers, outside the CMB field. -Starting in late December, the writing group will generate the final report based on the reviewer comments. A final workshop in Chicago which
22 //cmbpol.uchicago.edu Information ory Workshop, June 23-26, 2008 milab //astro.fnal.gov/cmb/welcome.html tematics Workshop, July 28-30, 8, Annapolis, MD //cmbpol.uchicago.edu/workshops/systematic2008 chnology Workshop, August , Boulder, CO //cmbpol.uchicago.edu/workshops/technology2008
23 e CMB is a unique property of the niverse. the past decade is any guide, it ould be wise to assume that the nformation it provides, beyond what ill come of the next generation of xperiments, will be important in ays we do not yet know.
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