4.7 Article

Resonant mode for gravitational wave detectors based on atom interferometry

期刊

PHYSICAL REVIEW D
卷 94, 期 10, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.94.104022

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资金

  1. National Science Foundation [PHY-1316706, PHY-1417295, PHY-1507160]
  2. U.S. Department of Energy [DE-SC0012012]
  3. W. M. Keck Foundation
  4. Simons Foundation [378243]
  5. Heising-Simons Foundation [2015-037, 2015-038]
  6. Direct For Mathematical & Physical Scien
  7. Division Of Physics [1316706] Funding Source: National Science Foundation
  8. U.S. Department of Energy (DOE) [DE-SC0012012] Funding Source: U.S. Department of Energy (DOE)

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We describe an atom interferometric gravitational wave detector design that can operate in a resonant mode for increased sensitivity. By oscillating the positions of the atomic wave packets, this resonant detection mode allows for coherently enhanced, narrow-band sensitivity at target frequencies. The proposed detector is flexible and can be rapidly switched between broadband and narrow-band detection modes. For instance, a binary discovered in broadband mode can subsequently be studied further as the inspiral evolves by using a tailored narrow-band detector response. In addition to functioning like a lock-in amplifier for astrophysical events, the enhanced sensitivity of the resonant approach also opens up the possibility of searching for important cosmological signals, including the stochastic gravitational wave background produced by inflation. We give an example of detector parameters which would allow detection of inflationary gravitational waves down to Omega(GW) similar to 10(-14) for a two-satellite space-based detector.

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