2. • This has been a great
week: great talks, great
venue, great people…
• Thank you, organizers,
staff and volunteers!
3. • This has been a great
week: great talks, great
venue, great people…
• Thank you, organizers,
staff and volunteers!
• I cannot possibly
discuss every talk.
Sorry!
15. Neutrino mass and mixing
Plot from H. Muryama/PDG
Neutrino physics enters
the era of precision
measurement,
yet there are still a lot of
know unknowns
(discoveries to be made)
2004
18. Solar neutrinos - Final SNO results
• Resolved solar neutrino problem
• Demonstrated flavor transformation
• consistent with LMA prediction
N. Barros
32. Reactor neutrinos and θ13
2-Detector mode (Far+Near)RENO
Double Chooz
sin2(2θ13) |Δmee2| x 10-3 eV2
Daya Bay 0.0841 ± 0.0027 ± 0.0019 2.50 ± 0.06 ± 0.06
RENO 0.086 ± 0.006 ± 0.005 2.61 ± 0.15 ± 0.09
Double Chooz 0.123 ± 0.023
Daya Bay
Gu, Choi, Vivier
33. Reactor neutrinos and θ13
2-Detector mode (Far+Near)RENO
Double Chooz
sin2(2θ13) |Δmee2| x 10-3 eV2
Daya Bay 0.0841 ± 0.0027 ± 0.0019 2.50 ± 0.06 ± 0.06
RENO 0.086 ± 0.006 ± 0.005 2.61 ± 0.15 ± 0.09
Double Chooz 0.123 ± 0.023
Daya Bay
Gu, Choi, Vivier
statistics limited
34. Reactor neutrino anomaly - I
Daya Bay
RENO
Double Chooz
All saw “bump” at ~5 MeV, similar
shape
Likely due to nuclear fission modeling
and not new neutrino properties
Gu, Choi, Vivier
64. KATRIN
AP
First light (2016.10) - beamline clear
83mKr (2017.07) Good performance
• Commissioning phase
• Rydberg H* atom background:
• Run and field optimization
• mβ ~ 240 meV
• 3H run to start in 2018
68. Considerations
• Preferably:
• high isotopic abundance
• high efficiency
• large mass
• long exposure
• low background
• good energy resolution
There is not an
obvious choice
of isotope or
detector
technology
79. IceCube - astrophysical neutrinos
Arguelles Delgado
Astrophysical neutrinos
New 6 year high energy starting
events result: softer spectrum,
consistent with one power law.
No astrophysical tau neutrinos
observed
80. Neutrino messengers — ANTARES/KM3Net
Excellent pointing
Constraints on the origin of the IceCube signal
81. In just 20 years…
• Our signals have become others’ backgrounds
82. In just 20 years…
• Our signals have become others’ backgrounds
• Track info to suppress directional
background
• Fine-grained nuclear emulsion
Vasina