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Dr Tomohiro Fujita (Geneva Uni./Kyoto Uni.)21/01/2019, 14:00
Identification of dark matter has been an outstanding problem in
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physics for decades, and axion (or axion like partciles) is its
candidate with great motivations. A number of observations and experiments have tried to detect axion by using the axion-photon conversion by assuming the axion is coupled to photon, while no signal yet to be found. In this talk, I will discuss new techniques to... -
Dr Wei Xue (CERN)21/01/2019, 14:45
In this talk, I will introduce a novel model to explain the small structure observations of galaxies. This model contains ultralight bosonic fields and heavy fermionic particles as dark matter. The second part of talk will revisit the idea of femtolensing of gamma ray bursts, which has been put forward as an exciting possibility to probe exotic astrophysical objects with masses below 10^−13...
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Dr Zhong-Zhi Xianyu (Harvard University)21/01/2019, 16:00
Abstract: Gravitational wave (GW) astronomy provides us a unique chance to probe invisible matter in the universe. In this talk we introduce several ways of probing dark ambient matter of compact binaries through GWs. We first present some analytical understanding of the distribution of binaries' orbital parameters and its relation to binaries' formation channels. Then, we describe how the...
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Dr Dražen Glavan (louvain-la-neuve university)21/01/2019, 16:45
The rapid expansion of inflationary universe amplifies microscopic linear quantum fluctuations of non-conformally coupled fields such as the minimally coupled massless scalar, and generates large superhorizon correlators. On the other hand, conformally coupled fields such as the photon are insensitive to the expansion itself. However, if the photon couples to the complex scalar the effect of...
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