Gravitational wave detection with optical lattice atomic clock

Researchers propose a space-based gravitational wave detector consisting of two spatially separated, drag-free satellites sharing ultra-stable optical laser light over a single baseline. Each satellite contains an optical lattice atomic clock, which serves as a sensitive, narrowband detector of the local frequency of the shared laser light. A synchronized two-clock comparison between the satellites will be sensitive to the effective Doppler shifts induced by incident gravitational waves (GWs) at a level competitive with other proposed space-based GW detectors, while providing complementary features. The detected signal is a differential frequency shift of the shared laser light due to the relative velocity of the satellites, and the detection window can be tuned through the control sequence applied to the atoms’ internal states. This scheme enables the detection of GWs from continuous, spectrally narrow sources, such as compact binary inspirals, with frequencies ranging from ~3 mHz – 10 Hz without loss of sensitivity, thereby bridging the detection gap between space-based and terrestrial optical interferometric GW detectors. Our proposed GW detector employs just two satellites, is compatible with integration with an optical interferometric detector, and requires only realistic improvements to existing ground-based clock and laser technologies.

The Harvard-Smithsonian Center for Astrophysics (CfA) has long been renowned for its laboratory work producing some of the best precision devices in the world. In particular are its timekeeping hydrogen-maser clocks, used by NASA to track its satellites as well as by radio astronomers around the world to make precision measurements of cosmic phenomena using Very Long Baseline Interferometry. The CfA maser group has continued to develop advanced clock technologies over the years, and to turn them into new tools to probe the heavens, including recently the so-called “laser-combs” for ultraprecise measurement of stellar velocity shifts induced by extrasolar planets.

CfA scientists Igor Pokovski, Nick Langellier, and Ron Walsworth and two colleagues have published a new GW detector concept to study in particular the low frequency GWs. Their technique precisely measures not the separation of the sensors but their minuscule motions via the Doppler effect as a gravitational waves passes by. The device uses a finely controlled laser and precise atomic clocks mounted in two satellites (unlike other space GW concepts that require three satellites, this system needs only two). The technology for this capability requires only realistic improvements to implement, and offers an important extension to current GW systems.

The recent detection of gravitation waves (GW) from the merger of two black holes of about thirty solar-masses each with the ground-based LIGO facility has generated renewed enthusiasm for developing even more sensitive measurement techniques. Ground-based GW instruments have widely spaced sensors that can detect sub-microscopic changes in their separation—better than one part in a billion trillion, They suffer, however, from the noise produced by small ground tremors—vibrations from natural or man-made sources that ripple through the precisely tuned detectors. The vibrations most difficult to compensate for are those that change relatively slowly, at frequencies around once a second or less, yet astronomers predict that GW sources producing these slow variations should be interesting and abundant, from compact stellar-mass binary stars to gravitational events in the early universe

Arxiv – Gravitational wave detection with optical lattice atomic clock

Further Research

Igor Pokovski publications

[15] P. Bosso, S. Das, I. Pikovski, and M. R. Vanner Amplified transduction of Planck-scale effects for quantum optical experiments
submitted [arXiv:1610.06796]

[14] S. Singh, L. A. De Lorenzo, I. Pikovski, and K. C. Schwab
Detecting continuous gravitational waves with superfluid 4He submitted [arXiv:1606.04980]

[13] I. Pikovski, M. Zych, F. Costa, and Č. Brukner Time Dilation in Quantum Systems and Decoherence New J. Phys. 19, 025011 (2017), [arXiv:1508.03296]

[12] S. Kolkowitz, I. Pikovski, N. Langellier, M. D. Lukin, R. L. Walsworth, and J. Ye
Gravitational wave detection with optical lattice atomic clocks
Phys. Rev. D 94, 124043 (2016), [arXiv:1606.01859]

[11] F. Armata, L. Latmiral, I. Pikovski, M. R. Vanner, Č. Brukner, and M. S. Kim
Quantum and Classical Phases in Optomechanics
Phys. Rev. A 93, 063862 (2016), [arXiv:1604.05679]

[10] I. Pikovski, and A. Loeb
Quantum coherent oscillations in the early universe Phys. Rev. D 93, 101302(R) (2016), [arXiv:1509.08895]
Selected for the Phys. Rev. D Kaleidoscope feature.

[9] L. Latmiral, F. Armata, M. G. Genoni, I. Pikovski, and M. S. Kim
Probing anharmonicity of a quantum oscillator in an optomechanical cavity
Phys. Rev. A 93, 052306 (2016), [arXiv:1602.03516]

[8] I. Pikovski, M. Zych, F. Costa, and Č. Brukner
Universal decoherence due to gravitational time dilation Nature Phys. 11, 668-672 (2015), [arXiv:1311.1095]
Nature Physics News and Views by A. Bassi – Gravity: Wanna be quantum

[7] R. Kaltenbeck et al.
Macroscopic quantum resonators (MAQRO): 2015 Update

EPJ Quantum Technology 3, 5 (2016), [arXiv:1503.02640].

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