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Planning begins on 'squeezed light' for LIGO-India

Sentinel Digital DeskBy : Sentinel Digital Desk

  |  3 April 2017 12:00 AM GMT

Kolkata, April 2: In the run-up to setting up LIGO in India by 2024, researchers are pushing boundaries of modern science to enhance sensitivity of detection of gravitatiol waves. They are, in fact, toying with quantum mechanics to “squeeze light”.

Squeezed light (a squeezed state of light) is a special form of light that is generated by tweaking quantum properties of light, to lower “noise” below the fundamental quantum limit. The resulting “quieter detector” can be harnessed for even more extreme precision and sensitivity of the gravitatiol wave detectors.

“Squeezed light will be used in Advanced LIGO (Laser Interferometer Gravitatiol Wave Observatory) by the early next decade. By the time LIGO-India comes up, US detectors will start using squeezed light (by 2022) and we will also be ready to start experiments with it,” Tarun Souradeep, spokesperson, LIGO-India Science, told IANS at the conclusion of the latest meeting on the project. The recently-concluded ‘LIGO-India: The Road ahead’ (LITRA-3) two-day meet at IUCAA-Pune, involved a discussion between the LIGO-India Science Magement Board, members of the LIGO Directorate (Dave Reitze, LIGO Director and Fred Raab, LIGO Associate Director), and prominent researchers from all over the country. Participants were from IIT Madras, IIT Delhi, IIT Kanpur, IISER Pune, CSIR-NPL, BITS-Pilani Goa, IIT Hyderabad, Saha Institute of Nuclear Physics and tiol Physical Laboratory. “We are making sure there are people who are taking up advanced areas of experimentation like squeezed light sources, so that we have all the technology for the RnD in LIGO-India,” explained Souradeep, also the senior professor at Inter-University Centre for Astronomy and Astrophysics, one of the three lead Indian institutions involved in implementing the collaborative LIGO-India project. He said IITs like the ones at Madras (Cheni), Delhi, Kanpur and IISERs Pune are taking up responsibilities related to quantum photonics, including squeezed light.

“Many of them are running smaller-scale projects on squeezed light. Many elements of LIGO are lab physics but the challenge is to scale it up from lab physics to the level of LIGO. It is like scaling up 100 times,” he explained. Some of the other issues on the table are seismic properties and the mitigation of associated noise of the shortlisted site where the observatory will be established and designing even more advanced laser sources and better optical coatings. (IANS)

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