GWEOS-2019 Pisa Workshop

Europe/Rome
Room N. 131 (Physics Department - Pisa University and INFN - Sezione di Pisa)

Room N. 131

Physics Department - Pisa University and INFN - Sezione di Pisa

Largo Bruno Pontecorvo, 3 - 56127 Pisa (Italy)
Ignazio Bombaci (University of Pisa and INFN Pisa) , Giancarlo Cella (INFN Pisa and Virgo Collaboration) , Cristiano Palomba (INFN ROMA1 and Virgo Collaboration)
Description

The idea of the workshop is to put together physicists with competences in gravitational waves, nuclear physics and neutron star physics to create a bridge between these communities and to foster future collaborations.

A large amount of time is allocated for discussions, and the style of the communications should be open to dialogue. Here is a list of issues we aim to discuss:

  • What kind of constraints on the equation of state (EOS) of matter at very high densities are allowed by the present and future GW detector sensitivities?

  • What are the most up to date theoretical models for the EOS?

  • Can neutron stars sustain long-lived large quadrupolar deformations?

  • What is the current state of the art for numerical simulations?

  • What are the more urgent theoretical challenges?

  • What are the most relevant analysis limitations?

  • How can we bring together GW and EM constraints?

  • What do we expect to gain with third-generation GW observatories for fundamental physics of matter at extreme densities?

Foreseen talks are on invitation only, but registration is open to everyone interested (within a numerical limit). Registrants are welcome to participate to the discussions.

We are happy to acknowledge the support of:

 

Registration
Registration form
50 / 50
Participants
  • Alejandro Kievsky
  • Alessandro Drago
  • Alessandro Nagar
  • Alice Boldrin
  • Andrea Bevilacqua
  • Andrea Maselli
  • Andrew Lawrence Miller
  • Anna Puecher
  • Atousa Pournaghi
  • Bruno Giacomazzo
  • Carla Signorini
  • Cristiano Palomba
  • Danny Laghi
  • Dario Grasso
  • Davide Vaccaro
  • Domenico Logoteta
  • Elena Pian
  • Elia Giliberti
  • Evgeni Kolomeitsev
  • Fiorella Burgio
  • Francesco Pegoraro
  • Giancarlo Cella
  • Hans Josef Schulze
  • Ian Harry
  • Ian Jones
  • Ignazio Bombaci
  • Konstantin Maslov
  • Leonardo Gualtieri
  • Magdalena Sieniawska
  • Mahmoud Elmasry
  • Margherita Fasano
  • Marie Anne Bizouard
  • Massimo Mannarelli
  • Matteo Breschi
  • Matteo Di Giovanni
  • Michal Bejger
  • Mihail Mintchev
  • Paolo Mazzali
  • Prasanta Char
  • Rainer Stiele
  • Roberto De Pietri
  • Rosana de Oliveira Gomes
  • Sabrina D'Antonio
  • Sebastiano Bernuzzi
  • Sebastien Guillot
  • stavros katsanevas
  • Steve Shore
  • Viviana Fafone
  • Walter Del Pozzo
  • Xisco Jimenez Forteza
  • Monday, 25 February
    • 09:00 09:20
      Registration 20m Room N. 131

      Room N. 131

      Physics Department - Pisa University and INFN - Sezione di Pisa

      Largo Bruno Pontecorvo, 3 - 56127 Pisa (Italy)
    • 09:20 09:30
      Welcome 10m Room N. 131

      Room N. 131

      Physics Department - Pisa University and INFN - Sezione di Pisa

      Largo Bruno Pontecorvo, 3 - 56127 Pisa (Italy)
    • 09:30 10:00
      LIGO-VIRGO results 30m Room N. 131

      Room N. 131

      Physics Department - Pisa University and INFN - Sezione di Pisa

      Largo Bruno Pontecorvo, 3 - 56127 Pisa (Italy)
      Speaker: Prof. Jo van den Brand (Nikhef - VU)
    • 10:00 10:30
      The TEONGRAV collaboration 30m Room N. 131

      Room N. 131

      Physics Department - Pisa University and INFN - Sezione di Pisa

      Largo Bruno Pontecorvo, 3 - 56127 Pisa (Italy)
      Speaker: Leonardo Gualtieri (ROMA1)
    • 10:30 11:00
      The NEUMATT collaboration 30m Room N. 131

      Room N. 131

      Physics Department - Pisa University and INFN - Sezione di Pisa

      Largo Bruno Pontecorvo, 3 - 56127 Pisa (Italy)
      Speaker: Alessandro Drago (FE)
    • 11:00 11:30
      Coffee break 30m Room N. 131

      Room N. 131

      Physics Department - Pisa University and INFN - Sezione di Pisa

      Largo Bruno Pontecorvo, 3 - 56127 Pisa (Italy)
    • 11:30 12:10
      The Equation of State of Nuclear Matter 40m Room N. 131

      Room N. 131

      Physics Department - Pisa University and INFN - Sezione di Pisa

      Largo Bruno Pontecorvo, 3 - 56127 Pisa (Italy)
      Speaker: Ignazio Bombaci (PI)
    • 12:10 12:50
      BNS mergers with modern microscopic nuclear EOS 40m Room N. 131

      Room N. 131

      Physics Department - Pisa University and INFN - Sezione di Pisa

      Largo Bruno Pontecorvo, 3 - 56127 Pisa (Italy)
      Speaker: Bruno Giacomazzo (TIFP)
    • 12:50 14:30
      Lunch break 1h 40m Room N. 131

      Room N. 131

      Physics Department - Pisa University and INFN - Sezione di Pisa

      Largo Bruno Pontecorvo, 3 - 56127 Pisa (Italy)
    • 14:30 15:10
      Extracting fundamental physics form GW signal 40m Room N. 131

      Room N. 131

      Physics Department - Pisa University and INFN - Sezione di Pisa

      Largo Bruno Pontecorvo, 3 - 56127 Pisa (Italy)
      Speaker: Walter Del Pozzo (P)
    • 15:10 15:50
      Isolated NS: results and perspectives 40m Room N. 131

      Room N. 131

      Physics Department - Pisa University and INFN - Sezione di Pisa

      Largo Bruno Pontecorvo, 3 - 56127 Pisa (Italy)
      Speaker: Dr Michal Bejger
    • 15:50 16:20
      Coffee break 30m Room N. 131

      Room N. 131

      Physics Department - Pisa University and INFN - Sezione di Pisa

      Largo Bruno Pontecorvo, 3 - 56127 Pisa (Italy)
    • 16:20 17:00
      GW emission from isolated NS: what we can learn? 40m Room N. 131

      Room N. 131

      Physics Department - Pisa University and INFN - Sezione di Pisa

      Largo Bruno Pontecorvo, 3 - 56127 Pisa (Italy)
      Speaker: Dr Ian Jones
    • 17:00 18:30
      Round table discussion (Panelists: M.A. Bizouard, G.F. Burgio, A. Nagar, C. Palomba) 1h 30m Room N. 131

      Room N. 131

      Physics Department - Pisa University and INFN - Sezione di Pisa

      Largo Bruno Pontecorvo, 3 - 56127 Pisa (Italy)
  • Tuesday, 26 February
    • 09:00 09:40
      TEOBResumS: efficient and accurate analytical waveform model for spin-aligned coalescing binaries 40m Auditorium (European Gravitational Observatory)

      Auditorium

      European Gravitational Observatory

      Via E. Amaldi 56021 S. Stefano a Macerata - Cascina (PI)

      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.

      Speaker: Alessandro Nagar (IHES)
    • 09:40 10:10
      Hyperons in Neutron Stars 30m Auditorium (European Gravitational Observatory)

      Auditorium

      European Gravitational Observatory

      Via E. Amaldi 56021 S. Stefano a Macerata - Cascina (PI)
      Speaker: Hans Josef Schulze (CT)
    • 10:10 10:40
      Crystalline Color Superconductors and GW from isolated Neutron Stars 30m Auditorium (European Gravitational Observatory)

      Auditorium

      European Gravitational Observatory

      Speaker: Massimo Mannarelli (LNGS)
    • 10:40 11:10
      Coffee break 30m European Gravitational Observatory

      European Gravitational Observatory

    • 11:10 11:50
      BNS mergers, NR simulations, e.m. counterparts 40m Auditorium (European Gravitational Observatory)

      Auditorium

      European Gravitational Observatory

      Speaker: Sebastiano Bernuzzi (PR)
    • 11:50 12:20
      BH-NS systems 30m Auditorium (European Gravitational Observatory)

      Auditorium

      European Gravitational Observatory

      Speaker: Ian Harry
    • 12:20 13:20
      Conclusion: general discussion (Panelists: G. Cella, W. Del Pozzo, R. De Pietri, A. Drago) 1h Auditorium (European Gravitational Observatory)

      Auditorium

      European Gravitational Observatory

    • 13:20 14:30
      Lunch Break 1h 10m European Gravitational Observatory

      European Gravitational Observatory

    • 14:30 15:30
      Visit to VIRGO 1h European Gravitational Observatory

      European Gravitational Observatory