Seminars
General information
The department is located at:
Ångström Laboratory, Polacksbacken, Lägerhyddsvägen 1.
Here's how to find us.
The seminars are available in several formats:
- Web: http://www.physics.uu.se/en/seminars/calendar
- iCal: http://www.physics.uu.se/sv/calendar/all/ical
- RSS-feed: http://www.physics.uu.se/en/seminars/upcoming/rss.xml
Information about Astronomy and Space Physics seminars
- Usual seminar time is Thursday, 14.00 sharp (45 min talk + 15 min discussion)
- Usual seminar room is Hiorters rum, floor 3, house 7
- Group meetings: Planets: Tue 15-16, IRFU: Wed 11-12, Galaxies: Fri 15-16, Stars: Fri 14-15
- Seminars at other Swedish institutes: Stockholm, Lund, Onsala
- Past and present IRFU seminars: 1996-present day
- Comments or inquiries regarding Astronomy and Space Physics seminars should be directed to the
seminar organizers (Andreas Korn and Eric Stempels).
Information about Nuclear and Particle Physics seminars
- Usual seminar time is Thursday, 15.15 (45-50 min talk + 10-15 min discussion)
- Usual seminar room is 12167, floor 2, southern end of house 1
- Comments or inquiries regarding Nuclear and Particle Physics seminars should be directed to the seminar organizer (Andrzej Kupsc and Richard Brenner).
Information about Theoretical Physics seminars
- Usual seminar time is Wednesday, 13.15-14.15
- Usual seminar room is Oseenska rummet, floor 3 house 7
- Past seminars: 2003-
- Comments or inquiries regarding the Theoretical Physics seminars should be directed to the seminar organizer (Thomas Klose)
Information about Applied Nuclear Physics seminars
- Comments or inquiries regarding the Applied Nuclear Physics seminars should be directed to the seminar organizer (Sophie Grape)
Information about Materials Theory seminars
- Usual seminar time is Friday, 14.15-15.00
- Usual seminar room is Å80101, floor 0 house 8
- Comments or inquiries regarding the "Materials Theory Friday Seminars" should be directed to the seminar organizer (Sumanta Bhandary)
Senast uppdaterad 2013-03-08 13:00.
Ansvarig: Webmaster
Kommande seminarier
The Aquarius stream is not really a stream at all
The Aquarius stream is a nearby (~5-10 kpc) stellar stream that was discovered as part of the RAVE spectroscopic survey. Since the group is co-moving, the default assumption is that it has been accreted onto the Milky Way by a disrupted satellite. Early indications from the RAVE spectra suggested there was a wide metallicity dispersion for the Aquarius group, whereas more recent follow-up observations have found very little dispersion in metallicity (~0.10 dex) and enhanced [Na/Fe], [Ni/Fe] abundance ratios.
Beam diagnostic instruments at 3rd and 4th generation light sources.
Ring and LINAC (FEL) based x-ray sources provide ultra-high brilliant photon beams to the experiments. These 3rd and 4th generation light sources require high resolution and reliable electron beam diagnostics to ensure very stable conditions at the experiments. This talk will discuss the different beam diagnostic needs of these accelerators and will compare theirs typical instruments. Examples from PETRAIII, the European XFEL and FLASH at DESY in Hamburg will be given.
Science in Business Interaction: A Study of the Collaboration between CERN and Swedish Companies
Susanne Åberg did defend her thesis in March 2013 with the title "Science in Business Interaction: A Study of the Collaboration between CERN and Swedish Companies"
"The aim of this thesis is twofold; to gain and understanding of how CERN, the European Organization for Nuclear Research, interacts with industry; and to gain an understanding of how CERN can become a resource for industry. Both parts of the purpose also have implications for the issue of CERN’s usefulness to industry.
