Study and experiment on the alternative technique of - - PowerPoint PPT Presentation

study and experiment on the alternative technique of
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Study and experiment on the alternative technique of - - PowerPoint PPT Presentation

Study and experiment on the alternative technique of frequencydependent squeezing generation with EPR entanglement for next generation of gravitational wave detectors. Mateusz Bawaj on behalf of Virgo squeezing team Noise sources in Adv


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Study and experiment

  • n the alternative technique
  • f frequency–dependent squeezing generation

with EPR entanglement for next generation of gravitational wave detectors.

Mateusz Bawaj on behalf of Virgo squeezing team

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SLIDE 2

09/09/2019 TAUP 2019

Noise sources in Adv Virgo

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SLIDE 3

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Improvement with FIS

GEO600: 6 dB LIGO: LLO 3.1 dB, LHO 2.2 dB

Advanced Virgo: 3.1 dB

(in collaboration with AEI)

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SLIDE 4

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Frequency dependent squeezing

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SLIDE 5

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Theoretical proposal

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Pros and cons

✗ intrinsic 3dB penalty ✗ more complicated detection setup with two homo-dyne detectors ✗ additional output mode cleaner is required

✔ no need for long fjlter cavity infrastructure ✔ variable phase rotation for various SRC confjguration

adjustable with idler detuning

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SLIDE 7

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EPR Squeezing Experiment

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SLIDE 8

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Improvement of Virgo detector

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SLIDE 9

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Conceptual design

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SLIDE 10

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Summary

Interesting theoretical proposal Experimental demonstration Work on the conceptual design

  • f the apparatus

On-going simulations of compatibility with Virgo

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SLIDE 11

09/09/2019 TAUP 2019

Acknowledgements: This project has received funding from the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No 734303 *Bawaj M.1, Barsuglia M.2, Bazzan M.3,4, Calloni E.5, Ciani G.3,4, Conti L.4, D’Angelo B.6,7, De Laurentis M.5, De Rosa R.5,Di Pace S.8,9, Fafone V.10,11, Garaventa B.6,7, Gemme G.7, Gennai A.12, Giacoppo L.10,11, Harms J.13,14, Khan I.13,11, Majorana E.8,9, Naticchioni L.8,9, Nguyen C.2, Passuello D.12, Prodi G.15, Ricci F.8,9, Rocchi A.11, Sequino V.7, Sorrentino F.7, Vardaro M.3,4, Zendri J.P.4 *mateusz.bawaj@pg.infn.it

1 – INFN Sezione di Perugia, I-06123 Perugia, Italy 2 – Laboratoire AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, F-75205 Paris Cedex 13, France 3 – Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy 4 – INFN Sezione di Padova, I-35131 Padova, Italy 5 – Università di Napoli “Federico II”, Complesso Universitario di Monte S.Angelo, I-80126 Napoli, and INFN Sezione di Napoli, Italy 6 – Università degli Studi di Genova, Dipartimento di Fisica, I-16146 Genova, Italy 7 – INFN Sezione di Genova, I-16146 Genova, Italy 8 – Università di Roma “La Sapienza”, I-00185 Roma,Italy 9 – INFN Sezione di Roma “ La Sapienza”, I-00185 Roma, Italy 10 – Università di Roma “Tor Vergata”, I-00133 Roma, Italy 11 – INFN Sezione di Roma “Tor Vergata”, I-00133 Roma, Italy 12 – INFN Sezione di Pisa, I-16146 Pisa, Italy 13 – Gran Sasso Science Institute, I-67100 L’Aquila, Italy 14 – INFN Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy 15 – Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, and INFN Sezione di Trento, Italy