Colloquium Prague ν17
from
Thursday, 2 November 2017 (06:50)
to
Friday, 3 November 2017 (20:00)
Monday, 30 October 2017
Tuesday, 31 October 2017
Wednesday, 1 November 2017
Thursday, 2 November 2017
08:00
Registration
Registration
08:00 - 09:00
09:00
Welcome
-
Rupert Leitner
(
Charles University (CZ)
)
Welcome
Rupert Leitner
(
Charles University (CZ)
)
09:00 - 09:10
09:10
Recent results from the Daya Bay experiment
-
Zeyuan Yu
(
Institute of High Energy Physics, China
)
Recent results from the Daya Bay experiment
Zeyuan Yu
(
Institute of High Energy Physics, China
)
09:10 - 09:45
09:45
RENO
-
Seon Hee Seo
(
Seoul National University (KR)
)
RENO
Seon Hee Seo
(
Seoul National University (KR)
)
09:45 - 10:20
10:20
CERN nu platform
-
Filippo Resnati
(
CERN
)
CERN nu platform
Filippo Resnati
(
CERN
)
10:20 - 10:55
10:55
Coffee Break
Coffee Break
10:55 - 11:15
11:15
KATRIN
-
Florian Fraenkle
(
Karlsruhe Institute of Technology
)
KATRIN
Florian Fraenkle
(
Karlsruhe Institute of Technology
)
11:15 - 11:50
11:50
Fermilab short baseline
-
Christos Touramanis
(
University of Liverpool (GB)
)
Fermilab short baseline
Christos Touramanis
(
University of Liverpool (GB)
)
11:50 - 12:25
12:25
T2K, T2HK
-
David Wark
T2K, T2HK
David Wark
12:25 - 13:10
13:10
Lunch
Lunch
13:10 - 14:15
Room: Cafeteria
14:15
NOvA
-
Mark Messier
(
IU
)
NOvA
Mark Messier
(
IU
)
14:15 - 14:50
14:50
IceCube and IceCube-Gen2
-
Justin Evans
(
University of Manchester (UK)
)
IceCube and IceCube-Gen2
Justin Evans
(
University of Manchester (UK)
)
14:50 - 15:25
The IceCube experiment, a cubic kilometre neutrino telescope, was built at the South Pole with the goal of observing high-energy neutrinos from beyond our solar system. This goal has been achieved with spectacular success, and now the collaboration aims to identify the sources of these interstellar neutrinos. At the heart of the IceCube detector a more densely instrumented region, called DeepCore, enables atmospheric neutrinos, with energies as low as 5 GeV, to be studied. These studies have led to a number of measurements of neutrino-oscillation phenomena, which will be the focus of my talk. I will present recent measurements of neutrino oscillation parameters and tau-neutrino appearance, and a search for sterile neutrinos. I will then talk about the future, outlining plans for the next phase of neutrino astronomy at the South Pole, IceCube-Gen2, and presenting the physics case, at both low and high energies, for this exciting new venture.
15:25
DUNE
-
Stefan Soldner-Rembold
(
University of Manchester (GB)
)
DUNE
Stefan Soldner-Rembold
(
University of Manchester (GB)
)
15:25 - 16:00
16:00
Coffee Break
Coffee Break
16:00 - 16:20
16:20
Global fits to neutrino oscillations: current status and robustness
-
Mariam Tórtola
(
IFIC, Valencia University/CSIC
)
Global fits to neutrino oscillations: current status and robustness
Mariam Tórtola
(
IFIC, Valencia University/CSIC
)
16:20 - 16:55
In this talk, I will summarize the current status of global neutrino oscillation analyses in the three-neutrino framework. I will also discuss some scenarios where the precise measurement of the neutrino oscillation parameters, such as theta_13 or the CP violation phase, could be significantly affected by the presence of neutrino physics beyond the Standard Model.
16:55
Double Beta Decay Theory
-
Fedor Šimkovic
(
Comenius University
)
Double Beta Decay Theory
Fedor Šimkovic
(
Comenius University
)
16:55 - 17:30
17:30
Prospects of direct observation of lepton number violation: the search for neutrinoless double beta decay
-
Bela Majorovits
(
MPI for Physics
)
Prospects of direct observation of lepton number violation: the search for neutrinoless double beta decay
Bela Majorovits
(
MPI for Physics
)
17:30 - 18:05
19:00
Social Dinner
Social Dinner
19:00 - 23:00
Friday, 3 November 2017
09:00
The JUNO detector
-
Marcos Dracos
(
Institut Pluridisciplinaire Hubert Curien (FR)
)
The JUNO detector
Marcos Dracos
(
Institut Pluridisciplinaire Hubert Curien (FR)
)
09:00 - 09:35
09:35
The Physics of JUNO
-
Gioacchino Ranucci
(
Istituto Nazionale di Fisica Nucleare
)
The Physics of JUNO
Gioacchino Ranucci
(
Istituto Nazionale di Fisica Nucleare
)
09:35 - 10:10
10:10
KNO
-
Seon Hee Seo
(
Seoul National University (KR)
)
KNO
Seon Hee Seo
(
Seoul National University (KR)
)
10:10 - 10:45
10:45
Coffee Break
Coffee Break
10:45 - 11:05
11:05
v at Cosmology
-
Michal Malinský
(
Charles University (CZ)
)
v at Cosmology
Michal Malinský
(
Charles University (CZ)
)
11:05 - 11:40
11:40
DANSS (Detector of reactor AntiNeutrino based on SolidState Scintillator)
-
Viacheslav Egorov
(
JINR
)
DANSS (Detector of reactor AntiNeutrino based on SolidState Scintillator)
Viacheslav Egorov
(
JINR
)
11:40 - 12:15
The detector (described in arXiv:1606.02896) is located at ~11 m from the core of industrial reactor (Kalinin Nuclear Power Plant, Russia) and is in operation for about 1 year, Looking for short-range neutrino oscillations. At the moment, together with ČVUT ÚTEF we construct a new version of the detector which could be installed at Temelin NPP (Czechia).
12:15
Closeout
-
David Wark
(
Oxford University / RAL
)
Closeout
David Wark
(
Oxford University / RAL
)
12:15 - 12:50
12:50
Lunch, Farewell
Lunch, Farewell
12:50 - 14:05
Room: Cafeteria