GWEOS-2019 Pisa Workshop
from
Monday, 25 February 2019 (08:00)
to
Tuesday, 26 February 2019 (18:00)
Monday, 25 February 2019
09:00
Registration
Registration
09:00 - 09:20
Room: Room N. 131
09:20
Welcome
Welcome
09:20 - 09:30
Room: Room N. 131
09:30
LIGO-VIRGO results
-
Jo van den Brand
(
Nikhef - VU
)
LIGO-VIRGO results
Jo van den Brand
(
Nikhef - VU
)
09:30 - 10:00
Room: Room N. 131
10:00
The TEONGRAV collaboration
-
Leonardo Gualtieri
(
ROMA1
)
The TEONGRAV collaboration
Leonardo Gualtieri
(
ROMA1
)
10:00 - 10:30
Room: Room N. 131
10:30
The NEUMATT collaboration
-
Alessandro Drago
(
FE
)
The NEUMATT collaboration
Alessandro Drago
(
FE
)
10:30 - 11:00
Room: Room N. 131
11:00
Coffee break
Coffee break
11:00 - 11:30
Room: Room N. 131
11:30
The Equation of State of Nuclear Matter
-
Ignazio Bombaci
(
PI
)
The Equation of State of Nuclear Matter
Ignazio Bombaci
(
PI
)
11:30 - 12:10
Room: Room N. 131
12:10
BNS mergers with modern microscopic nuclear EOS
-
Bruno Giacomazzo
(
TIFP
)
BNS mergers with modern microscopic nuclear EOS
Bruno Giacomazzo
(
TIFP
)
12:10 - 12:50
Room: Room N. 131
12:50
Lunch break
Lunch break
12:50 - 14:30
Room: Room N. 131
14:30
Extracting fundamental physics form GW signal
-
Walter Del Pozzo
(
P
)
Extracting fundamental physics form GW signal
Walter Del Pozzo
(
P
)
14:30 - 15:10
Room: Room N. 131
15:10
Isolated NS: results and perspectives
-
Michal Bejger
Isolated NS: results and perspectives
Michal Bejger
15:10 - 15:50
Room: Room N. 131
15:50
Coffee break
Coffee break
15:50 - 16:20
Room: Room N. 131
16:20
GW emission from isolated NS: what we can learn?
-
Ian Jones
GW emission from isolated NS: what we can learn?
Ian Jones
16:20 - 17:00
Room: Room N. 131
17:00
Round table discussion (Panelists: M.A. Bizouard, G.F. Burgio, A. Nagar, C. Palomba)
Round table discussion (Panelists: M.A. Bizouard, G.F. Burgio, A. Nagar, C. Palomba)
17:00 - 18:30
Room: Room N. 131
Tuesday, 26 February 2019
09:00
TEOBResumS: efficient and accurate analytical waveform model for spin-aligned coalescing binaries
-
Alessandro Nagar
(
IHES
)
TEOBResumS: efficient and accurate analytical waveform model for spin-aligned coalescing binaries
Alessandro Nagar
(
IHES
)
09:00 - 09:40
Room: Auditorium
will review the status of TEOBResumS, a freely available analytical waveform model, based on the effective one body approach (improved by numerical relativity simulations), to generate highly-accurate (and computationally inexpensive) time-domain (multipolar) waveforms for spin-aligned coalescing binaries. The model includes tidal interaction as well as EOS-dependent self-spin couplings (at high order) and is viable for both coalescing black holes through merger and ringdown or neutron stars (as well as mixed binaries) up to merger. Implications for data-analysis and in particularly its use on GW170817 are explicitly discussed.
09:40
Hyperons in Neutron Stars
-
Hans Josef Schulze
(
CT
)
Hyperons in Neutron Stars
Hans Josef Schulze
(
CT
)
09:40 - 10:10
Room: Auditorium
10:10
Crystalline Color Superconductors and GW from isolated Neutron Stars
-
Massimo Mannarelli
(
LNGS
)
Crystalline Color Superconductors and GW from isolated Neutron Stars
Massimo Mannarelli
(
LNGS
)
10:10 - 10:40
Room: Auditorium
10:40
Coffee break
Coffee break
10:40 - 11:10
11:10
BNS mergers, NR simulations, e.m. counterparts
-
Sebastiano Bernuzzi
(
PR
)
BNS mergers, NR simulations, e.m. counterparts
Sebastiano Bernuzzi
(
PR
)
11:10 - 11:50
Room: Auditorium
11:50
BH-NS systems
-
Ian Harry
BH-NS systems
Ian Harry
11:50 - 12:20
Room: Auditorium
12:20
Conclusion: general discussion (Panelists: G. Cella, W. Del Pozzo, R. De Pietri, A. Drago)
Conclusion: general discussion (Panelists: G. Cella, W. Del Pozzo, R. De Pietri, A. Drago)
12:20 - 13:20
Room: Auditorium
13:20
Lunch Break
Lunch Break
13:20 - 14:30
14:30
Visit to VIRGO
Visit to VIRGO
14:30 - 15:30