Mostrando 61 - 80 Resultados de 191 Para Buscar '"LIGO"', tiempo de consulta: 0.16s Limitar resultados
  1. 61
    “…Looking to the future, the major upgrades to LIGO (Advanced LIGO), Virgo (Advanced Virgo), LCGT and GEO600 (GEO-HF) will be completed over the coming years, which will create a network of detectors with the significantly improved sensitivity required to detect gravitational waves. …”
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    Online Artículo Texto
    Gravitational Wave Detection by Interferometry (Ground and Space)
  2. 62
    “…The recent Advanced LIGO and Advanced Virgo joint observing runs have not claimed a stochastic gravitational-wave background detection, but one expects this to change as the sensitivity of the detectors improves. …”
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    Simultaneous estimation of astrophysical and cosmological stochastic gravitational-wave backgrounds with terrestrial detectors
  3. 63
    “…We apply the delay in timing of FERMI GMB transient occurred in coincidence with gravitational waves event GW150914 observed by LIGO to constrain the size of the spherical brane-universe expanding in multi-dimensional space-time. …”
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    Size of Shell Universe in Light of FERMI GBM Transient Associated with GW150914
  4. 64
    por Barish, Barry C
    Publicado 1996
    “…The sources of gravitanional waves and techniques for detection will be presented, as well as the status and prospects for the LIGO project.…”
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    The detection of gravitational waves
  5. 65
    “…Gravitational interferometers such as the LIGO detectors capture cosmic events such as black hole mergers which happen at unknown times and of varying durations, producing time-series data. …”
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    Accelerating Recurrent Neural Networks for Gravitational Wave Experiments
  6. 66
    “…The first direct measurement of gravitational waves by the LIGO and Virgo collaborations has opened up new avenues to explore our Universe. …”
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    Challenges and Opportunities of Gravitational Wave Searches at MHz to GHz Frequencies
  7. 67
    por Jones, Robert
    Publicado 1996
    “…The aim is to show how individual developers can improve the quality of the software they produce while avoiding the conflict between the creative process of designing software and the organisational needs of large projects.The Laser Interferometer Gravitanional Wave Observatory (LIGO) is being constructed with a goal to detect these waves and then to use them as a new tool to explore and study The sources of gravitanional waves and techniques for detection will be presented, as well as the status and prospects for the LIGO project.…”
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    Software engineering: turning theory into practice
  8. 68
    “…Operating AION in a network with other gravitational wave detectors such as LIGO, Virgo and LISA would also offer many synergies.…”
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    AION: An Atom Interferometer Observatory and Network
  9. 69
    “…Upcoming results from LIGO-Virgo third observation run might reinforce or weaken these predictions.…”
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    The Evolution of Primordial Black Holes and their Final Observable Spins
  10. 70
    por Fidecaro, Francesco
    Publicado 2018
    “…This followed the detection of gravitational wave signals by the LIGO interferometers in 2015, which started the detailed study of highly curved space time.…”
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    The Virgo gravitational wave interferometer: status and perspectives
  11. 71
    por Amelino-Camelia, Giovanni
    Publicado 1999
    “…In particular, I find that the sensitivity level expected for the planned LIGO and VIRGO interferometers and for the next upgrade of the NAUTILUS resonant-bar detector corresponds to a white-noise level which can be naturally associated with the Planck length.…”
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    A testable description of space-time foam as a fundamental stochastic gravity-wave background
  12. 72
    “…We point out that the observed time delay between the detection of the signal at the Hanford and Livingston LIGO sites from the gravitational wave event GW150914 places an upper bound on the speed of propagation of gravitational waves, $c_{gw}\lesssim 1.7$ in the units of speed of light. …”
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    On constraining the speed of gravitational waves following GW150914
  13. 73
    “…Hence, we constrain the graviton mass using aLIGO and pulsar-timing observations (which give the most stringent bounds at present). …”
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    Online Artículo Texto
    Graviton propagation within the context of the D-material universe
  14. 74
    por Bassan, Massimo
    Publicado 2014
    “…Beside the VIRGO and GEO gravitational wave observatories in Europe and the two LIGOs in the United States, which have operated successfully during the past decade, further observatories are being completed (KAGRA in Japan) or planned (ILIGO in India). …”
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    First VESF School on Advanced Detectors for Gravitational Waves
  15. 75
    “…The observation of gravitational waves from the Laser Interferometer Gravitational-Wave Observatory (LIGO) event GW150914 may be used to constrain the possibility of Lorentz violation in graviton propagation, and the observation by the Fermi Gamma-Ray Burst Monitor of a transient source in apparent coincidence may be used to constrain the difference between the velocities of light and gravitational waves: $c_g - c_\gamma < 10^{-17}$.…”
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    Comments on Graviton Propagation in Light of GW150914
  16. 76
    “…Their sensitivity to mid-frequency gravitational waves may open a window on mergers of masses intermediate between those discovered by the LIGO and Virgo experiments and the supermassive black holes present in the cores of galaxies, as well as fundamental physics processes in the early Universe such as first-order phase transitions and the evolution of networks of cosmic strings.…”
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    Large-Scale Atom Interferometry for Fundamental Physics
  17. 77
    por Schilling, Govert
    Publicado 2017
    “…Govert Schilling takes readers to sites where these stories unfolded―including Japan’s KAGRA detector, Chile’s Atacama Cosmology Telescope, the South Pole’s BICEP detectors, and the United States’ LIGO labs. He explains the seeming impossibility of developing technologies sensitive enough to detect waves from two colliding black holes in the very distant universe, and describes the astounding precision of the LIGO detectors. …”
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    Ripples in spacetime: Einstein, gravitational waves, and the future of astronomy
  18. 78
    por Vaskonen, Ville, Veermäe, Hardi
    Publicado 2019
    “…This implies robust constraints on the PBH abundance in the range 1–100M⊙. We further show that LIGO/Virgo design sensitivity has the potential to reach the PBH mass range of 10-2–103M⊙. …”
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    A lower bound on the primordial black hole merger rate
  19. 79
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    Propostion d'expérience : mise en évidence du changement subi par le moment d'inertie des noyaux déformés dans les atomes mésiques par une mesure d'absorption critique
  20. 80
    por Kembhavi, Ajit, Khare, Pushpa
    Publicado 2020
    “…Also described are the LIGO detectors and the cutting edge technology that goes into building them, and the extremely accurate measurements that are needed to detect gravitational waves. …”
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    Gravitational waves: a new window to the Universe
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