XX Physics in Collision Conference
Lisbon, June 29 - July 1, 2000
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Presentation
Title:
"Neutrino Overview"
Session:
Electro-Weak
Author:
Gian Luigi Fogli
Institution:
Univ. of California Berkeley
Download:
PIC20-Gian.Luigi.Fogli.tgz
(HTML, 1.988MB)
Transparencies:
1:
Neutrino Oscillations: an Overview
2:
Introduction
3:
1. Present evidence
4:
2. The "Standard" 3
interpretation
5:
Parameters probed by oscillations
6:
Graphical representation of parameter space
7:
A remark
8:
3. 3
: atmospheric neutrinos
9:
SK zenithal distribution (
'99 data: 52kTy)
10:
Allowed regions in a three-flavour approach
11:
Allowed regions in a three-flavour approach
12:
Coupling Superkamiokande and CHOOZ
13:
Limits on U
2
e3
(
inconstrained)
14:
Best-fit distributions
15:
Progress in m
2
bounds for unconstrained 3
mixing
16:
Progress in constraining mixing
17:
Status of (m
2
,
,
) constraints
18:
A remark on LBL
19:
4. 3
oscillations: solar neutrinos
20:
Solar neutrino problem, 1999
21:
2
vacuum oscillations solution (
=0): total rates
22:
2
vacuum oscillations solution (
=0): SK spectrum
23:
2
vacuum oscillations solution (
=0)
24:
2
MSW solutions
25:
3
MSW solutions
26:
3
MSW solutions
27:
3
MSW solutions
28:
2
as a function of
(
m
2
and
unconstrained)
29:
3
MSW solutions
30:
Borexino
31:
Gallium Neutrino Observatory
32:
Example of solar + atmospheric combination
33:
Summary on colar
34:
3
summary
35:
5. The LSND signal: 4
oscillations
36:
Constraints on 4
mass/mixing schemes ...
37:
Two subcases
38:
6. Conclusions
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interpretation
inconstrained)
) constraints
2 as a function of 
m2 and 
unconstrained)