Monday, Feb 8, 2010
Monday Feb 8, 2010, 8:00 AM
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7:15 PM
America/Los_Angeles
C520 (Institute for Nuclear Theory (INT))
C520
Institute for Nuclear Theory (INT)
University of Washington Seattle, WA, USA
Description
Registration, Plenary session 1, 2, 3, 4 and working group meetings
Support
numass2010@physics.wisc.edu
Registration
INT office, 4th floor
INT office, 4th floor
Institute for Nuclear Theory (INT)
University of Washington Seattle, WA, USA
Plenary Session 1
C520
C520
Institute for Nuclear Theory (INT)
University of Washington Seattle, WA, USA
1
Welcome
Speaker
:
K.M. Heeger
Slides
2
Kinematic measurements
Speaker
:
R.G.H. Robertson
Slides
3
Neutrino mass from double beta decay experiments
Speaker
:
J.F. Wilkerson
Slides
4
Theory of neutrino mass and of double beta nuclear matrix elements
Speaker
:
P. Vogel
Slides
10:40 AM
coffee break
C520
C520
Institute for Nuclear Theory (INT)
University of Washington Seattle, WA, USA
Plenary Session 2
C520
C520
Institute for Nuclear Theory (INT)
University of Washington Seattle, WA, USA
5
Neutrino masses from oscillation experiments
Speaker
:
C. White
Slides
6
Neutrino mass and core collapse supernovae
Speaker
:
G. Fuller
Slides
7
Neutrino mass and weak lensing
Speaker
:
S. Dodelson
Slides
12:30 PM
lunch break
C520
C520
Institute for Nuclear Theory (INT)
University of Washington Seattle, WA, USA
Plenary Session 3
C520
C520
Institute for Nuclear Theory (INT)
University of Washington Seattle, WA, USA
8
Neutrino masses from CMB and large scale structure
Speaker
:
Y. Wong
Slides
9
Direct detection of relic neutrinos
Speaker
:
J. Formaggio
Slides
10
Neutrino masses and cosmic simulations
Speaker
:
M. Takada
Slides
11
Seeing cosmic neutrinos through CMB lenses
Speaker
:
B. Keating
Slides
12
Treatment of neutrino masses in the PDG
Speaker
:
R. Miquel
Slides
13
Working groups Q1-3: structure and tasks
Speaker
:
K.M. Heeger
Slides
4:10 PM
coffee break
C520
C520
Institute for Nuclear Theory (INT)
University of Washington Seattle, WA, USA
Working groups Q1, Q2, and Q3
C520 and others
C520 and others
Institute for Nuclear Theory (INT)
University of Washington Seattle, WA, USA
Q1, Q2 and Q3 work in parallel in different rooms
14
Q1 - direct measurements
C521
C521
Institute for Nuclear Theory (INT)
University of Washington Seattle, WA, USA
15
Q2 - double beta decay
C441
C441
Institute for Nuclear Theory (INT)
University of Washington Seattle, WA, USA
16
Q3 - astrophysics/cosmology
C520
C520
Institute for Nuclear Theory (INT)
University of Washington Seattle, WA, USA
Plenary Session 4
C520
C520
Institute for Nuclear Theory (INT)
University of Washington Seattle, WA, USA
17
Reconvene working groups
Questions and discussion
6:30 PM
end of session
C520
C520
Institute for Nuclear Theory (INT)
University of Washington Seattle, WA, USA