Session

Review

7 Dec 2021, 07:40
Online

Online

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  1. Tracy Slatyer (MIT)
    07/12/2021, 07:40

    The nature and origin of dark matter is one of the key unresolved questions of fundamental physics. Astrophysical and cosmological data provide powerful probes of dark matter properties, although to date no signal has been confirmed. I will give a status update on current constraints, future prospects, and open questions, including excesses/anomalies that are not yet fully understood.

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  2. Kathryn Zurek (Caltech)
    07/12/2021, 08:50
  3. Benjamin Safdi (UC Berkeley)
    08/12/2021, 07:00

    I will review the current status of the search for the QCD axion.

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  4. Anson Hook (Maryland)
    08/12/2021, 07:40

    I will review the current status of theoretical work on the QCD axion.

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  5. Irene Tamborra (NBI, Copenhagen)
    09/12/2021, 07:00

    Neutrinos are fascinating elementary particles heralding the dawn of the multi-messenger astronomy era. Neutrinos affect the stellar dynamics, drive the formation of new elements, and carry signatures of the yet mysterious physics ruling cosmic accelerators. Recent developments on neutrinos from cosmic sources will be reviewed together with detection prospects.

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  6. John Beacom (Ohio State)
    09/12/2021, 07:40

    Despite intensive searches, dark matter has not yet been discovered as a particle. Why not? Arguably, most searches are like looking for lost keys only under the lamppost, because that’s where we can see. I will assess how thoroughly we have really searched under the WIMP lamppost, point out opportunities for progress, and discuss the ultimate limitations of such searches. Then I will...

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  7. Masahiro Takada (Kavli IPMU, Tokyo)
    10/12/2021, 07:00

    In this talk I present the recent constraints on primordial black holes (PBHs) with microlensing methods, based on the Subaru Hyper Suprime-Cam (HSC) and the Optical Gravitational Lensing Experiment (OGLE) data. With Subaru HSC data, we obtained the tightest bound on the abundance of PBHs in the mass range of masses from asteroid to moon masses, but found a possible one candidate. We also...

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  8. Misao Sasaki (Kavli IPMU, Tokyo)
    10/12/2021, 07:40
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