POLARBEAR: Ultra-high Energy Physics with Measurements of Cosmic Microwave Background Polarization
POLARBEAR: Ultra-high Energy Physics with Measurements of Cosmic Microwave Background Polarization
批准号:
0618398
负责人:
Adrian Lee
金额:
$623.29万
依托单位国家:
美国
项目类别:
Continuing Grant
财政年份:
2007
资助国家:
美国
项目状态:
已结题
起止时间:
2007-09-01 至 2012-08-31
中文摘要
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英文摘要
AST 0618398LeeObservations of Cosmic Microwave Background (CMB) polarization are a powerful probe of cosmology and will eventually probe the standard model of physics at ultrahigh energy. With this award, Dr. Adrian Lee, University of California at Berkeley, will lead a new project called POLARBEAR (POLARization of the Background Radiation) which will use a dedicated telescope equipped with a powerful 1,200-bolometer array receiver to produce maps of CMB polarization with unprecedented accuracy. The most exciting possibility is that POLARBEAR will detect the signature of gravitational waves from the end of the inflationary period, 10-38 seconds after the Big Bang. If detected, these signals will provide an independent verification of the inflationary paradigm and test specific models for inflation. Another important scientific motivation is to characterize the gravitational lensing of the CMBpolarization. An accurate lensing measurement will yield constraints on Dark Energy. POLARBEAR can verify, or rule out, models with a strongly time-dependent Dark Energy equation of state w. In fact, POLARBEAR can provide information on w", the time derivative of w, which is comparable and complementary to that from a space-based supernovae search. The lensing signal is also sensitive to neutrino masses because massive neutrinos act as "hot" dark matter changing the formation of the lensing large scale structure. POLARBEAR introduces unprecedented levels of instrumental sensitivity and control of systematicerrors. The high sensitivity is achieved with an array of planar-antenna-coupled Transition-EdgeSensor (TES) bolometers operated at 250 mK. Dr. Lee and his colleagues have built and conducted tests of prototypes of these arrays. POLARBEAR's final configuration will include 1,200 bolometers distributed among three frequency bands at 90, 150, and 220 GHz.Members of the collaboration have played key roles on many of the best CMB experiments todate. They are also playing a key role in bringing the next generation of large TES focal planeinstruments. These experiments will be reaching maturity as POLARBEAR starts, and the collaboration members will be focused on building POLARBEAR. There will be significant international funding contributions from Canada on the readout electronics, from the UK on optical filters, and from France and the UK on data analysis. POLARBEAR is the most ambitious CMB polarization experiment to date, and it will explore theultimate limit of ground-based CMB polarimetry. POLARBEAR's unique combination of high sensitivity and stringent control of systematic errors will result in a search for inflationary gravitational waves over most of the experimentally accessible range.POLARBEAR will explore new technologies and methods that will carry forward to future CMB experiments such as NASA's CMBPOL mission. At UCSD, the team will connect POLARBEAR with the 'TRITONCAM' project that uses a radio telescope and polarimeter to teach physics to San Diego high school students.
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