ECU meeting: EPFL/CERN/UNIGE Joint Encounters
Wednesday 27 February 2019 -
09:00
Monday 25 February 2019
Tuesday 26 February 2019
Wednesday 27 February 2019
09:00
coffee
coffee
09:00 - 09:30
Room: 4/2-011 - TH common room
09:30
Novel Ways to Hunt Axion Dark Matter: Observation and Experiment
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Tomohiro Fujita
Novel Ways to Hunt Axion Dark Matter: Observation and Experiment
Tomohiro Fujita
09:30 - 10:30
Room: 4/3-006 - TH Conference Room
Identification of dark matter has been an outstanding problem for decades, and axion (or axion like particles) is one of the most popular dark matter candidates. 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 search for axion dark matter (ADM) by focusing on another phenomena, birefringence, which is caused by the same coupling. The polarimetry observation of protoplanetary disks puts the best constraint on ADM for fuzzy dark matter mass (m = 10^{-22}eV). I also propose a laser-cavity experiment which can improve the sensitivity by several orders of magnitude in the intermediate mass range (10^{-17}eV < m < 10^{-12}eV).
10:30
break
break
10:30 - 10:45
Room: 4/2-011 - TH common room
10:45
Dark Matter, First Light
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Katie Mack
Dark Matter, First Light
Katie Mack
10:45 - 11:30
Room: 4/3-006 - TH Conference Room
Dark matter forms the foundation for all cosmic structure, and its fundamental nature is one of science's most pressing enigmas. As we search for the most distant galaxies in the universe with radio and infrared observations, we are in a position to explore the particle physics of dark matter — the possibility of annihilation, decay, or other particle interactions — through its effects on early stars and galaxies. I will give an update on the quest to identify dark matter both in the lab and in the sky, major unsolved problems in dark matter theory, and how upcoming observations of the epoch of the first cosmic structures can be used to open a new window on the dark universe.
11:30
break
break
11:30 - 11:45
Room: 4/2-011 - TH common room
11:45
Why we should stop talking about the expansion of space
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Pierre Fleury
Why we should stop talking about the expansion of space
Pierre Fleury
11:45 - 12:30
Room: 4/3-006 - TH Conference Room
A popular stand about the interpretation of cosmic expansion is the following: « […] expansion redshift are produced by the expansion of space between bodies that are stationary in space. » [Harrison (2000)]. Most of us have been taught cosmology that way, and we naturally tend to replicate this message, notably in public outreach—think of the ubiquitous analogy of the inflating balloon. The same thing happens with gravitational waves, which are often referred to as « ripples in space-time », which stretch distances as they propagate. The concept of an « expanding space » is, however, in blatant contradiction with the fundamental principles of relativity. In this talk, I will argue that it is both unnecessary and dangerous for our intuitive understanding of the world. As such, we should abandon it.
12:30
lunch
lunch
12:30 - 13:00
Room: 501/R-014 Restaurant 1