advanced virgo and einstein telescope
play

Advanced Virgo and Einstein Telescope Bas Swinkels (Nikhef) 7 th - PowerPoint PPT Presentation

Advanced Virgo and Einstein Telescope Bas Swinkels (Nikhef) 7 th Belgium-Dutch GW meeting Groningen 29/05/2018 Advanced Virgo B. Swinkels AdVirgo & ET - Groningen 1 Advanced Virgo A lot has happened since the last meeting ...


  1. Advanced Virgo and Einstein Telescope Bas Swinkels (Nikhef) 7 th Belgium-Dutch GW meeting Groningen 29/05/2018 Advanced Virgo B. Swinkels – AdVirgo & ET - Groningen 1

  2. Advanced Virgo A lot has happened since the last meeting ... ● B. Swinkels – AdVirgo & ET - Groningen 2

  3. AdV commissioning before O2 Delayed due to various technical issues, main one was the repeated breaking of the monolithic fibers ● Decided to temporarily suspend mirrors with steel wires ● Commissioning was rushed to be able to join LIGO for the O2 science run ● Final big issue (aliasing of high frequency mirror modes) was solved only 3 weeks before the run ● Managed to join for just last month ... ● B. Swinkels – AdVirgo & ET - Groningen 3

  4. Advanced Virgo in O2 Participated for 24 days with 85% duty cycle, ~27 Mpc BNS range ● GW170814: first triple detection of a BBH ● GW170817: first detection of a BNS, low SNR in Virgo since it was ● in our blind spot, actually helped for the sky localization GW signal in coincidence with a GRB: start of multi-messenger ● astronomy, most observed event ever B. Swinkels – AdVirgo & ET - Groningen 4

  5. Post-O2: Monolithic supsension Problem identified and corrected : improved venting of vacuum system, fiber guards ● Mirrors re-installed with fused-silica fibers, should give theoretical increase from 30 to 50 Mpc ● Quality factor of violin modes lower than expected, suspect slightly increased thermal noise due to ear ● damage B. Swinkels – AdVirgo & ET - Groningen 5

  6. Other post-O2 upgrades Installed frequency independent squeezer built by AEI Hanover, beam into interferometer being aligned ● Replaced high-power laser amplifier (100W), up to 60 W available after Input Mode Cleaner ● New pre-mode-cleaner ● Installed seismometer arrays for testing Newtonian noise cancellation ● B. Swinkels – AdVirgo & ET - Groningen 6

  7. Post-O2 commissioning Increase of input power from 14 to 26.5 W, first use of Thermal Correction System ● Recovering of lock after suspension upgrade took bit longer than foreseen. Only recently back in low ● noise operation, best sensitivity so far 25 Mpc Unblocked External Injection Bench ● Goal: start O3 early next year with sensitivity of at least 60 Mpc ● Considerable contribution to commissioning effort by Nikhef members, see e.g. phase camera talk by ● Laura B. Swinkels – AdVirgo & ET - Groningen 7

  8. AdV+ upgrade 1 Mid-life upgrade of Advanced Virgo, transition form Advanced Virgo to Third Generation observatories, ● factor 2 improvement in sensitivity Phase 0 (120 Mpc): complete Advanced Virgo: ● monolithic suspensions: done, but improvement to be confirmed – high power laser: watch out for parametric instabilities, thermal effects – signal recycling: needs auxiliary green laser, or alternative lock acquisition strategy – Phase 1 (160 Mpc): ● frequency dependent squeezing: needs a ~300 m filter cavity – Newtonian news cancellation (see Boris’ talk for the sensors) – B. Swinkels – AdVirgo & ET - Groningen 8

  9. AdV+ upgrade 2 Phase 2 (300 Mpc): larger beams on larger, heavier mirrors ● Needs extensive R&D on coatings, upgrade of coating equipment, adaption of suspensions ● Exact details (optical design, mirror sizes) still TBD ● B. Swinkels – AdVirgo & ET - Groningen 9

  10. Einstein Telescope B. Swinkels – AdVirgo & ET - Groningen 10

  11. ET potential sites Birth of the ET collaboration, sign up for the letter of intent! http://www.et-gw.eu/index.php/letter-of-intent ● 3 candidate sites so far: ● BE/DE/NL: Liege/Aachen/Maastricht area – strong political support, interesting geology (see Soumen’s talk), lots of universities/high- tech companies nearby Italy: mountains in north of Sardinia – very uniform geology, dry, remote area Hungary: Matrá mountains, only limited seismic studies – B. Swinkels – AdVirgo & ET - Groningen 11

  12. ET prototype and other studies AEI 10 m CLIO 100 m (cryogenic) Will need to test key technology at prototype level before ET construction ● Recently submitted a pre-proposal for an InterReg project between provinces from Vlaanderen and south ● of NL, money is for facility only, need matched funding from others (NL groups, BE groups, province ...) ~10 m Fabry-Perot Michelson with cryogenic test masses ● Proposal so far is ‘for politicians only’, technical details to be decided soon ● More funding opportunities in the next years, also with Germany ● Urgent need for study of geologic/seismic feasibility of ET in the NL/BE/GE area ● B. Swinkels – AdVirgo & ET - Groningen 12

  13. Conclusions Joined O2 science run just in time, and what a time it was ... ● Post O2: short shutdown to finally install monolithic payloads, squeezer, high ● power laser Ambitious goal to reach 60 Mpc for O3 by the end of the year ● AdV+ upgrades: bridge between AdV and ET ● Time to prepare a serious bid to host ET in the NL/BE/DE area in the next years, ● need to act now B. Swinkels – AdVirgo & ET - Groningen 13

  14. End B. Swinkels – AdVirgo & ET - Groningen 14

Download Presentation
Download Policy: The content available on the website is offered to you 'AS IS' for your personal information and use only. It cannot be commercialized, licensed, or distributed on other websites without prior consent from the author. To download a presentation, simply click this link. If you encounter any difficulties during the download process, it's possible that the publisher has removed the file from their server.

Recommend


More recommend