Astronomy 596/496 NPA
Lecture 28, April 8
Spring 2019
Lecture Notes:
pdf file
Solar Neutrino Experiments
Radiochemical experiments
The pioneer:
Ray Davis
and the
Homestake Mine
experiment
GALLEX
experiment (
Gran Sasso
,
Italy
)
Scattering (water
Cerenkov
) experiments
Super-Kamiokande
(Japan)
beautiful high-energy atmospheric neutrino
event
;
grungier low-energy solar neutrino
event
Super-K
neutrino image
of the Sun
Sudbury Neutrino Observatory (SNO)
(Canada);
detector image
The 2002 Nobel Prize in Physics
The (Former) Solar Neutrino Problem
The problem:
8
B electron-neutrino deficit
The solution:
SNO
measures
the
flux
of
all
8
B neutrinos, and the
spectrum
of
8
B electron-neutrinos
The implications
new neutrino physics needed!
SSM bang on!
The laboratory test:
KamLAND
experiment
results
Borexino
(
7
Be neutrinos, and now
pp
too!)
the
2015 Nobel Prize in Physics
Future experiments:
Sanford Underground Research Facility
Lecture Archive