Welcome Room: Room N. 131

LIGO-VIRGO results

• Jo van den Brand (Nikhef - VU)

Room: Room N. 131

The TEONGRAV collaboration

• Leonardo Gualtieri (ROMA1)

Room: Room N. 131

The NEUMATT collaboration

• Alessandro Drago (FE)

Room: Room N. 131

The Equation of State of Nuclear Matter

• Ignazio Bombaci (PI)

Room: Room N. 131

BNS mergers with modern microscopic nuclear EOS

• Bruno Giacomazzo (TIFP)

Room: Room N. 131

Extracting fundamental physics form GW signal

• Walter Del Pozzo (P)

Room: Room N. 131

Isolated NS: results and perspectives

• Michal Bejger

Room: Room N. 131

GW emission from isolated NS: what we can learn?

• Ian Jones

Room: Room N. 131

Round table discussion (Panelists: M.A. Bizouard, G.F. Burgio, A. Nagar, C. Palomba) Room: Room N. 131

TEOBResumS: efficient and accurate analytical waveform model for spin-aligned coalescing binaries

• Alessandro Nagar (IHES)

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.

Hyperons in Neutron Stars

• Hans Josef Schulze (CT)

Room: Auditorium

Crystalline Color Superconductors and GW from isolated Neutron Stars

• Massimo Mannarelli (LNGS)

Room: Auditorium

BNS mergers, NR simulations, e.m. counterparts

• Sebastiano Bernuzzi (PR)

Room: Auditorium

BH-NS systems

• Ian Harry

Room: Auditorium

Conclusion: general discussion (Panelists: G. Cella, W. Del Pozzo, R. De Pietri, A. Drago) Room: Auditorium