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Niayesh Afshordi University of Waterloo. Kentaro Somiya Tokyo Institute of Technology. School of Science. Joey Key Assistant Professor of Physics. University of Washington Bothell. Pending formal confirmation of other members of the honour committee. GR22 and Amaldi13 in Valencia, Spain. Bill Weber University of Trento Italy. Clifford M. Edward K. Eva M. Meet all speakers. More info about location. Abstract : Recently there have been several proposals of low-energy precision experiments that can search for new particles, new forces, and the Dark Matter of the Universe in a way that is complementary to collider searches.

In this talk, I will present some examples involving ranging from atomic clocks, to astrophysical black holes accessible to LIGO. Abstract : The proximity of our Galaxy's center presents a unique opportunity to study a galactic nucleus with orders of magnitude higher spatial resolution than can be brought to bear on any other galaxy. After more than a decade of diffraction-limited imaging on large ground-based telescopes, the case for a supermassive black hole at the Galactic center has gone from a possibility to a certainty, thanks to measurements of individual stellar orbits.

The rapidity with which these stars move on small-scale orbits indicates a source of tremendous gravity and provides the best evidence that supermassive black holes, which confront and challenge our knowledge of fundamental physics, do exist in the Universe. This work was made possible through the use of speckle imaging techniques, which corrects for the blurring effects of the earth's atmosphere in post-processing and allowed the first diffraction-limited images to be produced with these large ground-based telescopes.

Further progress in high-angular resolution imaging techniques on large, ground- based telescopes has resulted the more sophisticated technology of adaptive optics, which corrects for these effects in real time. This has a strong impact in many other astrophysical fields, like fireballs detection, minor planet studies, the search for extra-solar planets, the monitoring of variable stars in our Galaxy, the study of active galactic nuclei, the detection and monitoring of supernovae, and the immediate follow-up of high-energy transients such as cosmic gamma-ray bursts, besides the search of neutrino and gravitational waves electromagnetic counterparts.

Last, but not least, space debris surveillance and tracking is another field of increasing interest. Educational aspects will be also covered. Related subject s :. Following the tradition of the previous NuSYM symposia, NuSYM is aimed to host synergies between the studies of nuclear structure, of nuclear reactions and of astrophysics, including new exciting ideas and all possible breakthroughs.

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Nuclear Physics. CGM Berlin Cosmic Controversies. Atomic and Molecular Physics. Warm Ionized Medium in Galaxies Workshop. One of the challenges of the LSST community is to optimize the scientific return of observations by preparing participants to source separation i.

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  6. Third Sino-Italian Workshop on Astrostatistics. Probability and Statistics, Game Theory. New Zealand Starlight Conference. Astrotourism, astrophotography, astronomy, lighting technology, artificial light at night, health impact of blue light, environmental impact of blue light, light pollution, LEDs, aesthetics of night sky. Galaxy Angular Momentum Alignment In the Spirit of Lyot White Dwarfs as probes of fundamental physics and tracers of planetary, stellar and galactic evolution - IAU Symposium From October 21 — 22nd we will hold the third brown dwarf to exoplanet connection conference on the campus of the University of Delaware.

    Gamma-ray Bursts in the Gravitational Wave Era Voyage workshop - Shaping the European Space Agency's space science plan for The TMT Science Forum is the prime opportunity to learn about the Thirty-Meter-Telescope, get an update on its design and construction, discuss its science capabilities, and become involved in shaping the observatory's future. Scintillometry Workshop Science with the Submillimeter Array: Present and Future. Courses and Events for Physics Students. MIST — Cosmic turbulence and magnetic fields : physics of baryonic matter across time and scales.

    Gravity drives the evolution of the universe, but the gas dissipative dynamics is a central, yet unsolved, issue in the theory of galaxy formation. Geophysics and Geology. First Spanish Meeting on Galaxy Clusters. As well as exposing participants to VLBI technique and analysis, this workshop also provides an excellent opportunity to identify core items, discuss about the role of Malaysia and future directions in the VLBI community, build up new collaborations among East Asia and worldwide astronomers, and increase the VLBI activities in the region.

    Plasma and Gas-discharge Physics, Nuclear Fusion. The school offers a broad training program including: - the theoretical aspects of the acceleration and propagation of non-thermal particles, - direct and indirect measurements of cosmic rays, - the role of cosmic rays in astrophysics and its place in multi-messenger astronomy and the understanding of dark matter, - two practical sessions on propagation models and their comparison to direct measurements, and data analysis with the future Cherenkov Telescope Array.

    Physics of acceleration and transport — Direct measures — Indirect measures — Cosmic rays and interstellar medium — Cosmic rays and dark matter. Universality: Turbulence Across Vast Scales. The goal of the workshop is to bring together experts in turbulence from the perspectives of astrophysics, plasma physics, biology, mathematics, atmospheric sciences, and experimental design. The next generation of analogue gravity experiments. Science at Low Frequencies VI.

    CoSyne — Cosmological Synergies in the upcoming decade.

    Physics, Astrophysics and Cosmology with Gravitational Waves | SpringerLink

    The coming decade of astrophysics and cosmology will be driven by a large number of missions which will explore the cosmos observing the sky through e. Cosmic microwave background, gravitational waves, large scale structure, line intensity mapping, standard candles.

    The School will cover topics relevant to theoretical and observational cosmology. Neutrino Cosmology, Non-linear perturbation theory, Testing dark energy with current and future observations, CMB polarisation and spectral distortions. Rocky Worlds: from the Solar System to Exoplanets. Non-vanishing neutrino masses and the existence of non-baryonic Dark Matter DM represent the only two firm observational evidences of new physics beyond the Standard Model SM. Nordic Institute of Theoretical Physics Nordita. The Cosmic Web in the Local Universe. This conference will bring together experts in cosmology, particle physics, and fundamental theory to address how and when the universe thermalizes following inflation, and the associated particle physics and dark matter phenomenology.

    Kavli-IAU Workshop — International co-ordination of multi-messenger transient observations in the s and beyond. The objective of this workshop is to explore the challenges in making international multi-messenger collaborations function and to draft a white paper with recommended best practice. Galaxy Quenching and Transformation throughout Cosmic Time.

    Magnetic Fields in the Universe 7. Dynamical Reconstruction of Galaxies. This international conference is part of a series of conferences that have been dedicated to the topic of Cosmic Flows over the last two decades: most recently in Queensland, Australia, in Marseille, France and in Quy Nhon, Vietnam.

    Flyby observations and related sciences, Onboard instruments with a special emphasis on cameras.


    Nordic Institute for Theoretical Physics Nordita. Understanding stellar convection is of crucial importance to many fields of stellar astrophysics. Cloud Academy II. The Physical Challenges of Astrostatistics. Astrostatistics is developing fast as astronomy is confronted to huge volumes of data.

    The two Fermi instruments have been surveying the high-energy sky since August Where the Star Formation Ends. Going into the s, cosmic large scale structure will be mapped with increasing detail by the next generation of observational facilities operating at various wavelengths radio, optical, infra-red and exploiting various techniques. Computational Physics and Numerical Simulation. Growing Black Holes: Accretion and Mergers. The interplay between ubiquitous dust, ice and gas in space knits an interesting tale from collapsing interstellar clouds to the formation of new stars, planets, moons and comets.

    Assembly and Evolution. The Sharpest Eyes on the Sky: A vision for high angular resolution astronomy.

    About the Series

    As general structure for the programme, we aim at discussing probes of cosmic expansion, tests of structure growth and at understanding the implications of combining them. This conference will synthesize recent observational discoveries of massive star clusters in nearby galaxies and the high-redshift universe. Mathematical Physics. The magnetized Galactic interstellar medium has become a main hindrance in the analysis of cosmological data. Cosmic microwave background, Large scale structure, Cosmic magnetism, Galactic astrophysics, Interstellar matter, Computational cosmology, component separation methods.

    Massive Stars Near and Far. This programme will bring together experts with complementary expertise in observation, theory, solar system and extrasolar planets to assess the current status of planet formation models, highlight problems in each formation stage, and explore the possibility of developing comprehensive models that can be applied to different planetary systems.

    Series in High Energy Physics, Cosmology and Gravitation

    Metrology and Instrumentation. SPIE — The international society for optics and photonics. Adaptive optics, exoplanets, Interferometry, infrared, polarimetry, telescope Instrumentation, spectrograph, spectroscopy, telescope, calibration, polarimetry, ELT, interferometry, wavefront sensing and distortion, diffractive optics. Extragalactic jets on all scales - launching, propagation, termination. Max Planck Institute for Astronomy, Heidelberg. Bosons Dark matter General relativity Gravitational wave detection Gravitational wave sources Gravitational waves Hypothetical particle physics models Particle dark matter Quantum fields in curved spacetime String phenomenology X ray astronomy.

    Cosmology - Gravitational Waves and Quantum Gravity

    Physical Systems. Astronomical black holes Axions Classical black holes Hypothetical gauge bosons Hypothetical scalars Quantum aspects of black holes. Mass Spin. Monte Carlo methods. Issue Vol. Authorization Required. Log In. Figure 1 Strain amplitude vs frequency for example black hole scalar cloud. Figure 2 Strain amplitude at different GW frequencies vs initial BH mass for fixed initial spin scalar cloud.

    Figure 3 Strain amplitude at different GW frequencies vs BH initial spin for fixed mass scalar cloud. Figure 4 Optimal strain frequency and amplitude vs initial BH mass for different initial spins scalar cloud. Figure 5 Optimal strain amplitude vs initial BH parameters scalar cloud. Figure 6 Signal growth and duration timescales for example BH scalar cloud. Figure 7 Superradiant-instability timescale scalar cloud.

    Figure 8 Signal duration timescale scalar cloud. Figure 9 HMM sample tracking paths. Figure 11 Sensitivity vs GW frequency for different detectors. Figure 12 Detection horizons for scalar clouds. Figure 13 [Horizon scaling with T drift ] Horizon scaling with T drift. Figure 14 Sky resolution. Sign up to receive regular email alerts from Physical Review D. Journal: Phys. X Rev. A Phys.