Probing the first stars and black holes in the early Universe with the Dark Ages Radio Explorer (DARE) |
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| Authors: | Jack O Burns J Lazio S Bale J Bowman R Bradley C Carilli S Furlanetto G Harker A Loeb J Pritchard |
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| Institution: | 1. Center for Astrophysics and Space Astronomy, Department of Astrophysical and Planetary Sciences, 593 UCB, University of Colorado Boulder, Boulder, CO 80309, USA;2. NASA Lunar Science Institute, NASA Ames Research Center, Moffett Field, CA 94035, USA;3. Jet Propulsion Laboratory, California Institute of Technology, M/S 138-308, 4800 Oak Grove Dr., Pasadena, CA 91109, USA;4. Space Sciences Laboratory, University of California at Berkeley, Berkeley, CA 94720, USA;5. Arizona State University, Department of Physics, P.O. Box 871504, Tempe, AZ 85287-1504, USA;6. National Radio Astronomy Observatory, 520 Edgement Road, Charlottesville, VA 22903, USA;g National Radio Astronomy Observatory, P.O. Box O, 1003, Lopezville Road, Socorro, NM 87801-0387, USA;h University of California at Los Angeles, Department of Physics and Astronomy, Los Angeles, CA 90095-1547, USA;i Center for Astrophysics, 60 Garden St., MS 51, Cambridge, MA 02138, USA |
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| Abstract: | A concept for a new space-based cosmology mission called the Dark Ages Radio Explorer (DARE) is presented in this paper. DARE’s science objectives include: (1) When did the first stars form? (2) When did the first accreting black holes form? (3) When did Reionization begin? (4) What surprises does the end of the Dark Ages hold (e.g., Dark Matter decay)? DARE will use the highly-redshifted hyperfine 21-cm transition from neutral hydrogen to track the formation of the first luminous objects by their impact on the intergalactic medium during the end of the Dark Ages and during Cosmic Dawn (redshifts z = 11–35). It will measure the sky-averaged spin temperature of neutral hydrogen at the unexplored epoch 80–420 million years after the Big Bang, providing the first evidence of the earliest stars and galaxies to illuminate the cosmos and testing our models of galaxy formation. DARE’s approach is to measure the expected spectral features in the sky-averaged, redshifted 21-cm signal over a radio bandpass of 40–120 MHz. DARE orbits the Moon for a mission lifetime of 3 years and takes data above the lunar farside, the only location in the inner solar system proven to be free of human-generated radio frequency interference and any significant ionosphere. The science instrument is composed of a low frequency radiometer, including electrically-short, tapered, bi-conical dipole antennas, a receiver, and a digital spectrometer. The smooth frequency response of the antennas and the differential spectral calibration approach using a Markov Chain Monte Carlo technique will be applied to detect the weak cosmic 21-cm signal in the presence of the intense solar system and Galactic foreground emissions. |
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| Keywords: | Cosmology: first stars dark ages reionization Radio lines: general Instrumentation: detectors |
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