Lutz Köpke und Mainz Person-Info 

( Ich bin Lutz Köpke)
(1 - 42 von 73
)

HAP Dark Matter ( September 2015)Indico@KIT

indico.scc.kit.edu
... Lutz Köpke (JGU Mainz), Marek Kowalski (HU Berlin, DESY Zeuthen), Gernot Maier (DESY Zeuthen), Uwe Oberlack (JGU Mainz), Martin Pohl (U Potsdam, DESY Lutz Köpke (JGU Mainz), Marek Kowalski (HU Berlin, DESY Zeuthen), Gernot Maier (DESY Zeuthen), Uwe Oberlack (JGU Mainz), Martin Pohl (U Potsdam, DESY ...

P-ONE virtual collaboration meeting ( December 2020)Home | CERN

indico.cern.ch
WOM status and data - Lutz Koepke (University of Mainz) Lutz Koepke (Universität Mainz) Lutz Koepke (). P-ONEDec20.pdf. 11:15, --- Tacos and tequila break ... WOM status and data - Lutz Koepke (University of Mainz) Lutz Koepke (Universität Mainz) Lutz Koepke (). P-ONEDec20.pdf. 11:15, --- Tacos and tequila break ...

SN neutrinos at the crossroads: astrophysics, oscillations ...FBK ECT

indico.ectstar.eu
Lutz Köpke (Johannes Gutenberg University Mainz). LutzKoepkeTrentoTalkshort.pptx SN neutrinos at JUNO. Speaker: Prof. Shun Zhou (Institute of High Energy ... Lutz Köpke (Johannes Gutenberg University Mainz). LutzKoepkeTrentoTalkshort.pptx SN neutrinos at JUNO. Speaker: Prof. Shun Zhou (Institute of High Energy ...

The next galactic supenova with the IceCube observatoryUppsala universitet

indico.uu.se
Lutz Köpke. Mainz Uppsala. Page 2. about 2 supernovae y in our galaxy. (45% probability in 30 years) energy release (R core. =106 m → R. NS. =104 m). Lutz Köpke. Mainz Uppsala. Page 2. about 2 supernovae y in our galaxy. (45% probability in 30 years) energy release (R core. =106 m → R. NS. =104 m).
+1