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  • richardmitnick 11:06 pm on January 27, 2021 Permalink | Reply
    Tags: "GEO600 reaches 6 dB of squeezing", , German-British instrument mitigates quantum noise effects better than any gravitational-wave detector before., Gravitational wave detectors, , ,   

    From MPG Institute for Gravitational Physics [MPG Institut für Gravitationsphysik] (Albert Einstein Institut) (DE): “GEO600 reaches 6 dB of squeezing” 

    From MPG Institute for Gravitational Physics [MPG Institut für Gravitationsphysik] (Albert Einstein Institut) (DE)

    January 27, 2021
    Media contact
    Dr. Benjamin Knispel
    Press Officer AEI Hannover
    +49 511 762-19104
    benjamin.knispel@aei.mpg.de

    Dr. James Lough
    Junior Scientist/Postdoc
    +49 511 762-17122
    james.lough@aei.mpg.de

    Dr. Christoph Affeldt
    Junior Scientist/Postdoc
    +49 511 762-2210
    christoph.affeldt@aei.mpg.de

    Prof. Dr. Karsten Danzmann
    Director
    Tel +49 511 762-2356
    Fax +49 511 762-5861
    karsten.danzmann@aei.mpg.de

    German-British instrument mitigates quantum noise effects better than any gravitational-wave detector before.

    Gravitational waves cause tiny length changes in the kilometer-size detectors of the international network (GEO600, KAGRA, LIGO, Virgo). The instruments use laser light to detect these effects and are so sensitive that they are fundamentally limited by quantum mechanics. This limit manifests as an ever-present background noise which can never be fully removed and which overlaps with gravitational-wave signals. But one can change the noise properties – using a process called squeezing – such that it does not disturb the measurements as much. Now, GEO600 researchers have achieved the strongest squeezing ever seen in a gravitational-wave detector. They lowered the quantum mechanical noise by up to a factor of two. This is a big step to third-generation detectors such as the Einstein Telescope and Cosmic Explorer. The GEO600 team is confident to reach even better squeezing in the future.

    Depiction of the ASPERA Albert Einstein Telescope, Albert Einstein Institute Hannover and Max Planck Institute for Gravitational Physics and Leibniz Universitat Hannover.

    GEO600 listens to a part of the Universe eight times larger

    1
    GEO600 background noise measurements. The horizontal axis shows the frequency, the vertical axis the strength of the detector noise at these frequencies. The lower the curves are, the less noise is present and the better gravitational waves can be measured. The blue curve shows the noise without the squeezed light source, the red curve shows the noise with the squeezed light source. The improvements occur mainly at high frequencies. Credit: Max Planck Institute for Gravitational Physics.

    2
    Inside the central building of the gravitational-wave detector GEO600. The unique squeezed-light source can be seen in the middle at the bottom of the picture. Credit: Max Planck Institute for Gravitational Physics.

    The team from the Max Planck Institute for Gravitational Physics (Albert Einstein Institute; AEI) and the Institute for Gravitational Physics at Leibniz University Hannover, together with partners at Cardiff University and University of Glasgow lowered the quantum background noise by a factor of 2, an achievement the scientists call a squeezing level of 6 dB.

    “We have focused on optimizing and characterizing the squeezed-light source at GEO600 and its interface to the detector. Compared to a detector without squeezing the observable volume of the Universe has now increased by a factor of 8 at high frequencies. This could help improve our understanding of neutron stars,” says Dr. James Lough, lead scientist for GEO600 and first author of the publication that appeared in Physical Review Letters.

    The research team achieved the new record with newly designed and custom-made optical components and by optimizing the optical setup of the squeezed-light source and how its output is fed into the detector.

    Pioneer work at GEO600

    “The German-British GEO600 team members are squeezed light pioneers. We have been routinely using squeezed light since 2010 and have been the only instrument in the world to do so until the start of O3 in April 2019,” explains Dr. Christoph Affeldt, GEO600 operations manager. “The custom-made squeezed-light source for GEO600 was developed and built at the AEI in Hannover. Several GEO600 PhD students together with squeezing experts at AEI have made this record possible.“

    Key to achieving ever better squeezing levels is a tight and lossless integration of the “squeezer” into the detector, because of the fragile nature of squeezed light. This is where the efforts of the team were focused recently. While squeezing can potentially increase the sensitivity of GEO600 by a lot, even the smallest loss on its way into the detector can degrade it. This way, many small incremental improvements can result in a large plus in sensitivity.

    On the way to third-generation detectors

    “The international community is currently planning the third generation of gravitational-wave detectors: the European Einstein Telescope and Cosmic Explorer in the US. Both will need even higher levels of squeezing than the impressive results we obtained. GEO600 is in the ideal position to further optimize this technology,” says Prof. Karsten Danzmann, director at the AEI and director of the Institute for Gravitational Physics at Leibniz Universität Hannover. “We are confident that at GEO600 we can reach 10 dB, the level of squeezing required for future gravitational-wave detectors.”

    See the full article here.

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    Stem Education Coalition

    MPG Institute for Gravitational Physics [MPG Institut für Gravitationsphysik] (Albert Einstein Institut) (DE) is the largest research institute in the world specializing in general relativity and beyond. The institute is located in Potsdam-Golm and in Hannover where it is closely related to the Leibniz Universität Hannover.

     
  • richardmitnick 12:02 pm on September 3, 2018 Permalink | Reply
    Tags: A new line of technical equipment in order to dramatically improve gravitational wave detectors, A small glass cell containing a cloud of 100 million caesium atoms, Boosting gravitational wave detectors with quantum tricks, , Gravitational wave detectors, ,   

    From Niels Bohr Institute: “Boosting gravitational wave detectors with quantum tricks” 

    University of Copenhagen

    Niels Bohr Institute bloc

    From Niels Bohr Institute

    03 September 2018
    Eugene Polzik, professor and head of the Center for Quantum Optics, Quantop at the Niels Bohr Institute, University of Copenhagen
    Phone: +45 2338 2045
    Email: polzik@nbi.dk

    Gravitational wave detectors: Niels Bohr Institute scientists are convinced they can expand space surveillance using a small glass cell filled with caesium atoms.

    2
    Eugene Polzik and Farid Khalili from LIGO collaboration and Moscow State University, have recently published in the scientific journal Physical Review Letters how they can improve gravitational wave detectors. Photo: Ola J. Joensen

    A group of scientists from the Niels Bohr Institute (NBI) at the University of Copenhagen will soon start developing a new line of technical equipment in order to dramatically improve gravitational wave detectors.

    Gravitational wave detectors are extremely sensitive and can e.g. register colliding neutron stars in space. Yet even higher sensitivity is sought for in order to expand our knowledge about the Universe, and the NBI-scientists are convinced that their equipment can improve the detectors, says Professor Eugene Polzik: “And we should be able to show proof of concept within approximately three years”.

    If the NBI-scientists are able to improve the gravitational wave detectors as much as they “realistically expect can be done”, the detectors will be able to monitor and carry out measurements in an eight times bigger volume of space than what is currently possible, explains Eugene Polzik: “This will represent a truly significant extension”.

    Polzik is head of Quantum Optics (Quantop) at NBI and he will spearhead the development of the tailor made equipment for gravitational wave detectors. The research – which is supported by the EU, the Eureka Network Projects and the US-based John Templeton Foundation with grants totaling DKK 10 million – will be carried out in Eugene Polzik’s lab at NBI.

    A collision well noticed

    News media all over the world shifted into overdrive in October of 2017 when it was confirmed that a large international team of scientists had indeed measured the collision of two neutron stars; an event which took place 140 million light years from Earth and resulted in the formation of a kilonova.

    The international team of scientists – which also included experts from NBI – was able to confirm the collision by measuring gravitational waves from space – waves in the fabric of spacetime itself, moving at the speed of light. The waves were registered by three gravitational wave detectors: the two US-based LIGO-detectors and the European Virgo-detector in Italy.


    VIRGO Gravitational Wave interferometer, near Pisa, Italy

    Caltech/MIT Advanced aLigo Hanford, WA, USA installation


    Caltech/MIT Advanced aLigo detector installation Livingston, LA, USA

    Cornell SXS, the Simulating eXtreme Spacetimes (SXS) project

    Gravitational waves. Credit: MPI for Gravitational Physics/W.Benger-Zib

    ESA/eLISA the future of gravitational wave research

    1
    Skymap showing how adding Virgo to LIGO helps in reducing the size of the source-likely region in the sky. (Credit: Giuseppe Greco (Virgo Urbino group)

    See also https://sciencesprings.wordpress.com/2017/10/16/from-ucsc-a-uc-santa-cruz-special-report-neutron-stars-gravitational-waves-and-all-the-gold-in-the-universe/

    2
    Caesium atoms contained in a spin-protecting cell are expected to enhance the sensitivity of Gravitational Waves Detectors. Photo: Ola J. Joensen

    “These gravitational wave detectors represent by far the most sensitive measuring equipment man has yet manufactured – still the detectors are not as accurate as they could possibly be. And this is what we intend to improve”, says Professor Eugene Polzik.

    How this can be done is outlined in an article which Eugene Polzik and a colleague, Farid Khalili from LIGO collaboration and Moscow State University, have recently published in the scientific journal Physical Review Letters. And this is not merely a theoretical proposal, says Eugene Polzik:

    “We are convinced this will work as intended. Our calculations show that we ought to be able to improve the precision of measurements carried out by the gravitational wave detectors by a factor of two. And if we succeed, this will result in an increase by a factor of eight of the volume in space which gravitational wave detectors are able to examine at present”.

    A small glass cell

    In July of last year Eugene Polzik and his team at Quantop published a highly noticed article in Nature – and this work is actually the very foundation of their upcoming attempt to improve the gravitational wave detectors.

    3
    If laser light used to measure motion of a vibrating membrane (left) is first transmitted through an atom cloud (center) the measurement sensitivity can be better than standard quantum limits envisioned by Bohr and Heisenberg. Photo: Bastian Leonhardt Strube and Mads Vadsholt

    The article in Nature centered on ‘fooling’ Heisenberg’s Uncertainty Principle, which basically says that you cannot simultaneously know the exact position and the exact speed of an object.

    This has to do with the fact that observations conducted by shining light on an object inevitably will lead to the object being ‘kicked’ in random directions by photons, particles of light. This phenomenon is known as Quantum Back Action (QBA) and these random movements put a limit to the accuracy with which measurements can be carried out at the quantum level.

    The article in Nature in the summer of 2017 made headlines because Eugene Polzik and his team were able to show that it is – to a large extent – actually possible to neutralize QBA.

    And QBA is the very reason why gravitational wave detectors – that also operate with light, namely laser light – “are not as accurate as they could possibly be”, as professor Polzik says.

    Put simply, it is possible to neutralize QBA if the light used to observe an object is initially sent through a ‘filter’. This was what the article in Nature described – and the ‘filter’ which the NBI-scientists at Quantop had developed and described consisted of a cloud of 100 million caesium atoms locked-up in a hermetically closed glass cell just one centimeter long, 1/3 of a millimeter high and 1/3 of a millimeter wide.

    The principle behind this ‘filter’ is exactly what Polzik and his team are aiming to incorporate in gravitational wave detectors.

    4
    PhD student Tulio Brasil, postdoctoral fellow Michael Zugenmaier and Professor Eugene Polzik in front of the future site of the experiment. Foto: Ola J. Joensen

    In theory one can optimize measurements of gravitational waves by switching to stronger laser light than the detectors in both Europe and USA are operating with. However, according to quantum mechanics, that is not an option, says Eugene Polzik:

    “Switching to stronger laser light will just make a set of mirrors in the detectors shake more because Quantum Back Action will be caused by more photons. These mirrors are absolutely crucial, and if they start shaking, it will in fact increase inaccuracy”.

    Instead, the NBI-scientists have come up with a plan based on the atomic ‘filter’ which they demonstrated in the Nature article: They will send the laser light by which the gravitational wave detectors operate through a tailor made version of the cell with the locked-up atoms, says Eugene Polzik: “And we hope that it will do the job”.

    See the full article here .


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    Stem Education Coalition

    Niels Bohr Institute Campus

    The Niels Bohr Institute (Danish: Niels Bohr Institutet) is a research institute of the University of Copenhagen. The research of the institute spans astronomy, geophysics, nanotechnology, particle physics, quantum mechanics and biophysics.

    The Institute was founded in 1921, as the Institute for Theoretical Physics of the University of Copenhagen, by the Danish theoretical physicist Niels Bohr, who had been on the staff of the University of Copenhagen since 1914, and who had been lobbying for its creation since his appointment as professor in 1916. On the 80th anniversary of Niels Bohr’s birth – October 7, 1965 – the Institute officially became The Niels Bohr Institute.[1] Much of its original funding came from the charitable foundation of the Carlsberg brewery, and later from the Rockefeller Foundation.[2]

    During the 1920s, and 1930s, the Institute was the center of the developing disciplines of atomic physics and quantum physics. Physicists from across Europe (and sometimes further abroad) often visited the Institute to confer with Bohr on new theories and discoveries. The Copenhagen interpretation of quantum mechanics is named after work done at the Institute during this time.

    On January 1, 1993 the institute was fused with the Astronomic Observatory, the Ørsted Laboratory and the Geophysical Institute. The new resulting institute retained the name Niels Bohr Institute.

    The University of Copenhagen (UCPH) (Danish: Københavns Universitet) is the oldest university and research institution in Denmark. Founded in 1479 as a studium generale, it is the second oldest institution for higher education in Scandinavia after Uppsala University (1477). The university has 23,473 undergraduate students, 17,398 postgraduate students, 2,968 doctoral students and over 9,000 employees. The university has four campuses located in and around Copenhagen, with the headquarters located in central Copenhagen. Most courses are taught in Danish; however, many courses are also offered in English and a few in German. The university has several thousands of foreign students, about half of whom come from Nordic countries.

    The university is a member of the International Alliance of Research Universities (IARU), along with University of Cambridge, Yale University, The Australian National University, and UC Berkeley, amongst others. The 2016 Academic Ranking of World Universities ranks the University of Copenhagen as the best university in Scandinavia and 30th in the world, the 2016-2017 Times Higher Education World University Rankings as 120th in the world, and the 2016-2017 QS World University Rankings as 68th in the world. The university has had 9 alumni become Nobel laureates and has produced one Turing Award recipient

     
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