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From Cosmochemistry to Solar Neutrinos

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Presentation on theme: "From Cosmochemistry to Solar Neutrinos"— Presentation transcript:

1 From Cosmochemistry to Solar Neutrinos
From Cosmochemistry to Solar Neutrinos A Retroperspective on the Occasion of Till Kirsten's 80th Birthday Manfred Lindner 33 plenary parallel =125 talks ca slides sec. ==> ca. 1.5 sec / slide 15 seconds for every 10 slides M. Lindner, MPIK From Cosmochemistry to Solar Neutrinos MEDEX'13, JUne 11-14, 2013

2 The roots of Astroparticle Physics @MPIK
Archeometry .... Cosmochemistry Aus: Wolfgang Gentner Festschrift zum 100. Geburtstag M. Lindner, MPIK From Cosmochemistry to Solar Neutrinos

3 From Cosmochemistry to Solar Neutrinos
Tektites Meteorites Historic materials (coins) Moon rock KTB rock samples …hard work ... no fun :-) M. Lindner, MPIK From Cosmochemistry to Solar Neutrinos

4 Low Background Physics
Chosmochemistry expertise  extremely useful for basic science with very rare events  neutrino physics double beta decay neutrino-less double beta decay neutrino mass solar neutrinos: GALLEX/GNO M. Lindner, MPIK From Cosmochemistry to Solar Neutrinos

5 From Cosmochemistry to Solar Neutrinos
GALLEX/GNO A great achievement!  clear n-deficit beyond solar modelling uncertainties …was fully appreciated only later (calibration, others) deserves more recognition! M. Lindner, MPIK From Cosmochemistry to Solar Neutrinos

6 From Cosmochemistry to Solar Neutrinos
Today (since 2006) division - builds on past expertise - improved methods see e.g. talks by C. Buck and H. Simgen M. Lindner, MPIK From Cosmochemistry to Solar Neutrinos

7 From Cosmochemistry to Solar Neutrinos
Theory and Experiment GERDA I+II (Borexino) STEREO Double Chooz neutrino phenomenology dark matter model building flavour physics EW symmetry breaking hot thermal Universe XENON100, XENON1T + new things… GIOVE CONUS XENOnT + R&D... M. Lindner, MPIK From Cosmochemistry to Solar Neutrinos

8 Very recent: Direct Detection Results (SI)
New XENON1T result from 34 live days Strongest exclusion limit: 7.7×10–47cm2 at 35 GeV/c2 Additional > 60 days of data already acquired, growing --> stay tuned! M. Lindner, MPIK From Cosmochemistry to Solar Neutrinos

9 End of 2018: XENON1T  XENONnT
M. Lindner, MPIK From Cosmochemistry to Solar Neutrinos

10 From Cosmochemistry to Solar Neutrinos
Happy birthday Till! Enjoy the workshop M. Lindner, MPIK From Cosmochemistry to Solar Neutrinos

11 Modulation of Electronic Recoils in XENON100
477 life days (48kg*year) aquired ; improved signal & bckg. modelling  DAMA/LIBRA signal 5.7s away  leptophilic models excluded source of modulation not understood Future: New NaI Projects to directly check DAMA  clarify modulation  new projects: SABRE, COSINUS, COSINE-100, ANAIS, KIMS-NaI, DM-Ice M. Lindner, MPIK 29th Recontre de Blois 2017


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