From the Muon Puzzle in cosmic-ray induced air showers to the LHC
Central seminar room, library building
ARI Institute Colloquium
Dorit Glawion
TeV Observations of Radio Galaxies
ARI Moenchhofstrasse 12-14, Seminarraum 1
16:15
Teilchen-Tee
Christof Gattringer
Lattice field theory with worldlines and worldsheets (PRETALK for students at 15:30 h)
Institut für Theoretische Physik, Phil12;SR106
Friday, 26 April 2019
16:15
SFB1225 ISOQUANT
Matthias Weidemüller
Light-matter interactions with atomic giants (Ring Lecture
Institut für Theoretische Physik, INF
17:00
Physikalisches Kolloquium
Prof. Michael Hesse
Heliophysics
KIP, INF 227, Otto-Haxel-Hörsaal
Monday, 29 April 2019
09:30
Special Seminar
Shuyuan Hu
Noise effects on the characterization of attosecond pulses
Bothe lab, seminar room
11:15
ITA "blackboard" Colloquium
Andrew Magalich
Lyman-alpha forest as a diagnostic for Warm Dark Matter
Philosophenweg, 12, 106
16:30
Particle and Astroparticle Theory Seminar
Prof. Susanne Westhoff (U. Heidelberg, ITP)
Long-lived Particles and Dark Matter
Library Building, Central Seminar Room
Tuesday, 30 April 2019
11:00
Astrophysics Seminar
Dr. Adriano Ingallinera, Univ. Palermo, Italy
Preparing to the ASKAP Galactic science: the SCORPIO project
Central seminar room, library building
SKA precursors are going to revolutionize our view of the Milky Way and we have to get prepared for that. ASKAP is the Australian SKA Pathfinder and EMU is the largest radio survey ever designed at the planned depth of 10 μJy/beam. In such a context, I present the SCORPIO project, a pathfinder survey of EMU, originally covering a ∼5-square-degree patch of the Galactic plane and now extended to ∼40 square degrees thanks to the first ASKAP early science observations. After a brief summary of the scientific and technical goals of this survey, I present the ASKAP early science observations of SCORPIO, carried out in January and November 2018 at 912 and 1600 MHz. I highlight the surprising capability of ASKAP to image wide fields toward the Galactic plane, focusing on its impact to the Galactic science. In particular I will stress its contribution to fields like the study of supernova remnants (SNRs), which are of interest for the gamma astronomy community. In the SCORPIO field we in fact observed at least 23 previously unidentified sources that we are proposing as SNR candidates, more than doubling the number of SNRs in SCORPIO known from the literature. I will give a panoramic view of the analysis we are performing on these sources and on the final goals of the projects we are involved in, in particular of the Italian "PRIN" project "gamma-prop" aimed at addressing the CTA science.
Kosmologie und Elementarteilchenphysik
Nevenko Bilic
Tachyon inflation in a holographic braneworld
Institut für Theoretische Physik, Phil16;SR
11:15
Seminar Theoretische Quantendynamik
Prof. Jian-Xing Li, Xi'an Jiaotong University, China
Ultrarelativistic electron and positron beam polarization in single-shot interaction with an ultraintense laser pulse
Seminarraum, Bothe Lab
16:15
Heidelberg Joint Astronomical Colloquium
Bryan M. Gaensler
Magnets in the Sky
Philosophenweg 12, großer Hörsaal
Thursday, 2 May 2019
11:15
Teekolloquium
Dino Jaroszynski, University of Strathclyde, Glasgow
Towards attosecond radiation sources based on laser-plasma accelerators
Grosser Hoersaal/Big Lecture Hall (library)
ARI Institute Colloquium
Trifon Trifonov
nn
ARI Moenchhofstrasse 12-14, Seminarraum 1
16:15
Teilchen-Tee
Thomas Konstandin
Implications of cosmological phase transitions (PRETALK for students at 15:30 h)
