1–5 Jul 2019
Faculty of Physics, University of Warsaw
Europe/Warsaw timezone

Session

Beyond I

1 Jul 2019, 08:00
Faculty of Physics, University of Warsaw

Faculty of Physics, University of Warsaw

conference hall 0.03, Faculty of Physics, University of Warsaw ul. Pasteura 5, 02-093 Warszawa Poland

Conveners

Beyond I

  • Yi Wang (afternoon)
  • Chunshan Lin (morning)

Description

Monday session

Presentation materials

There are no materials yet.

  1. Dr Chunshan Lin
    01/07/2019, 08:55
  2. Prof. Andrzej Królak (the leader of Polgraw-Virgo group)
    01/07/2019, 09:00

    Detection of gravitational wave signals from mergers of black holes and neutron stars is one the most important discoveries of this century. I shall briefly present the phenomenon of gravitational radiation as predicted by Einstein's general relativity. I shall describe gravitational wave detectors and
    methods of analyzing gravitational wave data. I shall review the observations made during...

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  3. Marek Lewicki (Kings College London)
    01/07/2019, 09:45
    contributed talk

    I will discuss efficiency factors for the production of gravitational waves through bubble collisions and plasma-related sources in strong phase transitions, and the conditions under which the bubble collisions can contribute significantly to the signal. I will also show that generically the sound-wave period is much shorter than a Hubble time leading to a reduction of GW signal produced by...

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  4. Qingwen Wang
    01/07/2019, 10:05
    contributed talk

    Exotic compact objects (ECOs) produce the same initial event detected by LIGO-Virgo collabo-ration as classical black holes (BHs), but various quantum gravity models feature the different following echoes. In particular, we investigate the echoes from the fluctuation-dissipation theorem [1, 2], which changes the dispersion relationship near the (would-be) horizon and results in a Boltzmann...

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  5. Dr Camilo Garcia Cely (DESY)
    01/07/2019, 10:25
    contributed talk

    A rather minimal possibility is that dark matter consists of the gauge bosons of a spontaneously broken symmetry. I will discuss the possibility of detecting the gravitational waves produced by the phase transition associated with such breaking. Concretely, I will focus on the scenario based on an 𝑆𝑈(2)_D group and argue that it is a case study for the sensitivity of future gravitational wave...

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  6. Prof. Misao Sasaki (Kavli IPMU, the University of Tokyo)
    01/07/2019, 11:15
  7. Prof. David Wands
    01/07/2019, 14:00

    Quantum fluctuations play an essential role in the dynamics and phenomenology of inflation in the very early universe. Usually quantum fluctuations during inflation are studied perturbatively (often linearly) about a fixed classical background, but in the stochastic approach quantum fluctuations on small scales provide a stochastic contribution to the non-perturbative classical evolution on...

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  8. Prof. Celine Boehm
    01/07/2019, 14:45

    The presence of dark matter strongly suggests that the laws of Physics as we know them are incomplete. In this talk I will summarise the directions which have been explored to determine the nature of dark matter (as well as their motivations), and discuss how future cosmological and astronomy surveys will help us to progress in this field.

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  9. Tim Morris (Southampton University)
    01/07/2019, 15:30
    contributed talk

    The Wilsonian renormalization group (RG) requires Euclidean signature. The conformal factor of the metric then has a wrong-sign kinetic term, which has a profound effect on its RG properties. In particular around the Gaussian fixed point, it supports a Hilbert space of renormalizable interactions involving arbitrarily high powers of the gravitational fluctuations. These interactions are...

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  10. Prof. Yi-fu Cai (University of Science and Technology of China)
    01/07/2019, 16:20

    In this talk I will briefly introduce the present understanding about the cosmic acceleration at present from the perspective of phenomenological study. I will review the latest observational status of the late-time cosmic acceleration and then depict how to do the model building of dynamical dark energy. Afterwards, I will also give an introduction to a type of torsional based modified...

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  11. Prof. Arttu Rajantie
    01/07/2019, 17:05

    When extrapolated to high energies, the Standard Model of particle physics predicts that the current vacuum state is metastable. Its predicted decay rate is currently extremely low, but it would have been much higher in the early Universe. Therefore the fact that the Universe survived its first moments places constraints on both the cosmological history and on particle physics. I will discuss...

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  12. Dr Stephen Stopyra (University College London)
    01/07/2019, 17:50
    contributed talk

    If the Standard Model vacuum is metastable, bubbles that form expand and convert the entire vacuum into a true vacuum state incompatible with observations. It is sometimes argued, however, that true vacuum bubbles forming during inflation are 'inflated away' and thus pose no danger to the present day universe, even if they form. I will argue that this point of view is incorrect - while the...

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  13. Miguel Escudero (King's College London)
    01/07/2019, 18:10
    contributed talk

    Within the framework of $\Lambda$CDM, the local determination of the Hubble constant disagrees -- at the 4.4$\sigma$ level -- with that inferred from the very accurate CMB observations by the Planck satellite. This clearly motivates the study of extensions of the standard cosmological model that could reduce such tension. Proposed extensions of $\Lambda$CDM that reduce this so-called Hubble...

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  14. contributed talk
  15. contributed talk
  16. contributed talk
  17. Dr Stephen Stopyra
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