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Bottom-Up Cross-Cutting Workshop “JENAS Initiative: Gravitational Wave Probes of Fundamental Physics”

→ Europe/Rome
Physics Department - Aula Amaldi (Marconi Building) (Sapienza University of Rome)

Physics Department - Aula Amaldi (Marconi Building)

Sapienza University of Rome

Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
Paolo Pani (Istituto Nazionale di Fisica Nucleare), Tetyana Galatyuk (TU Darmstadt / GSI)
Descrizione

We are excited to announce the first Bottom-Up Cross-Cutting Workshop of the JENAS Initiative “Gravitational Wave Probes of Fundamental Physics”, to be held at Sapienza University of Rome on Feb, 12-16 2024.

Città Universitaria La Sapienza | Turismo Roma

 

La Sapienza University of Rome - Pava Education

 

This will be the kick-off event that will shape the organization of our cross-cutting initiative, getting all members involved from the very beginning of this effort.

In this spirit, only the main broad topics of the workshop have been fixed, which are those discussed in this manifesto. The entire workshop structure and concrete topics has emerged from the bottom up, based on the feedback from the community

List of burning questions identified by the community.

To remain up-to-date with this and other initiatives, please subscribe to our mailing list: https://lists.infn.it/sympa/info/gwfundphys 

 

Working Groups:

  • WG1: Matter under extreme conditions
  • WG2: Nuclear and atomic physics and their role in multi-messenger astronomy
  • WG3: Fundamental problems in high-energy and gravitational physics
  • WG4: GWs & Cosmology
  • WG5: Synergies between particle accelerators and GWs

 

List of invited speakers & Conveneers:

Niayesh Afshordi (CAN)

Michalis Agathos (UK)

Andreas Bauswein (DE)

Diego Blas (ES)

Richard Brito (PT)

Katy Clough (UK)

Pippa Cole (IT)

Maximilian Dax (DE)

Gabriele Franciolini (CH)

Ettore Majorana (IT)

Cristiano Palomba (IT)

Krisztian Peters (DE)

Ira Rothstein (USA)

Alberto Sesana (IT)

Nils Schöneberg (ES)

Jan Steinheimer (DE)

Sarah Vigeland (USA)

 

 

Scientific Secretariat: Alessandra Curto  
Organizing Committee: Tetyana Galatyuk, Paolo Pani

on behalf of the Steering Committee: 
Sven Bernitt, Gianfranco Bertone, Vitor Cardoso, Roberto Emparan, Tetyana Galatyuk, Tanja Hinderer, Aleksi Kurkela, Ann-Cecilie Larsen, Marlene Nahrgang, Samaya Nissanke, Paolo Pani, Rafael Porto, Antonio Riotto, Stephan Rosswog

Support: This event is supported by INFN, JENAS, NuPECC, EMMI and Sapienza.

         Istituto nazionale di fisica nucleare - Wikipedia                   Joint ECFA – NuPECC – APPEC Activities » APPEC

 

UniRoma1 Università La Sapienza di Roma | Guida di ateneo - UnidTest   

   Meeting of the APPEC General Assembly » APPEC       



 

poster.pdf
Dr. Alessandra Curto
  • lunedì 12 febbraio
    • Registration Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
      Coordinatore: Alessandra Curto
    • 12:45
      Welcome Coffee Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
    • 1
      Welcome & Scope of the Workshop Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
      Relatori: Paolo Pani (Istituto Nazionale di Fisica Nucleare), Tetyana Galatyuk (TU Darmstadt / GSI)
      GWPFP JENAS Workshop (2).pdf
    • 2
      The QCD equation of state from Heavy ion collisions and neutron star mergers: Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)

      In this talk I will give a short overview on the current status and challenges in the exploration of dense QCD matter. While in relativistic heavy ion collisions, experiment and theory have been struggling for three decades to get a quantitative understanding of the QCD phase diagram. Only recently, new experimental programs allowed for significant progress. At the same time, the observation of gravitational waves from binary neutron star mergers has opened new venues in the study of dense QCD matter. Based on state-of-the-art models from both communities I intend to show the areas of overlap and opportunities for HIC and BNSM (with a short detour to core-collapse supernovae). In addition I plan to discuss open challenges and give some comments on what we can expect to learn from BNSM and what we should not expect to learn.

      Relatore: Jan Steinheimer-Froschauer (Frankfurt Institute for Advanced Studies)
      JENAS_24.pdf
    • 3
      Pions, hyperons and quark matter in neutron star mergers Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)

      We discuss recent calculations investigating the detailed
      impact of various "non-nucleonic" degrees of freedom in neutron star
      mergers. Pions are neglected in equation of state tables for merger
      simualtions but might actually occur in neutron star matter. We quantify
      their potential impact on the obseravbles of neutron star mergers. We
      describe a weak but potentially measurable signature of hyperons in
      neutron star mergers. Finally, we discuss the effects of deconfined
      quark matter.

      Relatore: Andreas Bauswein (GSI Darmstadt)
      talk_Rome2024.pdf
    • 15:15
      Coffee Break Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
    • WG1: Matter under extreme conditions: Overview and contributed talks Aula Cabibbo (Fermi Building)

      Aula Cabibbo (Fermi Building)

      Sapienza University of Rome

      https://maps.app.goo.gl/Nh2fQMCQFZx92hfv8
    • 18:20
      Wine & Cheese Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
  • martedì 13 febbraio
    • 10
      The Status of Analytical Theory: Methods and Bench Marks Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
      Relatore: Ira Rothstein
      Rome.pdf
    • 11
      Strong gravity as a probe of physics beyond GR and the Standard Model Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)

      I will discuss how GW probes could identify modifications to GR and the presence of new particles beyond the Standard Model. I will focus on how numerical simulations in strong gravity regimes can help us to understand and identify such signatures.

      Relatore: Katy Clough
      JENAS_RomeFeb24.pdf
    • 10:15
      Coffee Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
    • WG2: Nuclear and atomic physics and their role in multi-messenger astronomy: Overview and contributed talks Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
      • 12
        Overview by Conveners
        Relatori: Jan Steinheimer-Froschauer (Frankfurt Institute for Advanced Studies), Joachim Stroth (Goethe University Frankfurt)
        summary_WG2.pdf
      • 13
        Nonequilibrium evolution of quarkonium inside the Quark Gluon Plasma
        Relatore: Antonio Vairo
        Roma24.pdf
      • 14
        Nuclear physics inputs for neutron stars and nucleosynthesis simulations
        Relatore: Guilherme Grams
        GGramstalk_GWfundPhys-Fev24.pdf
      • 15
        NMMA: A nuclear-physics and multi-messenger astrophysics framework to analyze binary neutron star mergers
        Relatore: Nina Kunert (Institute for Physics and Astronomy, University of Potsdam, D-14476 Potsdam, Germany)
        Kunert_Romeconf.pdf
        video_nuclearconstraintapp.mp4
      • 16
        Decoding the phase structure of QCD via particle production at high energy
        Relatore: Anton Andronic (University of Munster)
        therm_roma24.pdf
    • 13:00
      Group picture Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
    • 13:00
      Lunch break Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
    • 17
      Ultralight bosons and gravitational waves: theory and observations Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
      Relatori: Cristiano Palomba (Istituto Nazionale di Fisica Nucleare), Richard Brito
      brito_JENAS.pdf
      palomba_ULDM_GW_observations.pdf
    • 18
      Quantum spacetime in the sky: from the horizon to the vacuum Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)

      I will discuss two aspects of the quantum fluctuations of vacuum spacetime that can be probed in gravitational wave (GW) observatories. The first is the quantum fluctuations near the horizon that lead to (stimulated) Hawking emission (a.k.a. echoes) AND multipolar deformation of Kerr geometry. The second is an irreducible noise in the GW detectors due to the quantum fluctuations of spacetime geometry. These are both (potential) manifestations of a UV/IR coupling that is inevitable in any non-perturbative theory of quantum gravity.

      Relatore: Niayesh Afshordi
      Rome_Feb_2024.pdf
    • 16:00
      Coffee Break Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
    • WG3: Fundamental problems in high-energy and gravitational physic: Overview and contributed talks Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
      • 19
        Overview by Conveneers
        Relatori: David Keitel (UIB), Elisa Maggio (Max Planck Institute for Gravitational Physics, Albert Einstein Institute, Potsdam)
        WG3 Overview.pdf
      • 20
        The ringdown of spinning horizonless compact objects
        Relatore: Elisa Maggio (Max Planck Institute for Gravitational Physics, Albert Einstein Institute, Potsdam)
        JENAS sapienza.pdf
      • 21
        Black holes as point particles: from amplitudes to self-force
        Relatore: Riccardo Gonzo (University of Edinburgh)
        Talk_Rome.pdf
      • 22
        Rotating metrics from scattering amplitudes in arbitrary dimensions
        Relatore: Claudio Gambino (Istituto Nazionale di Fisica Nucleare)
        Sapienza 24.pdf
      • 23
        Quantum Gravity Effects on Dark Matter and Gravitational Waves
        Relatore: Rishav Roshan (University of Southampton)
        Talk_Rishav.pdf
  • mercoledì 14 febbraio
    • 24
      Searching for Nanohertz Gravitational Waves with Pulsar Timing Arrays Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)

      Pulsar timing arrays are sensitive to low-frequency gravitational waves with periods of months to decades. They do so by precisely timing a collection of millisecond pulsars, whose extremely stable rotation makes them ideal for measuring perturbations in spacetime. Gravitational waves induce correlations in the pulse arrival times that follows a characteristic pattern known as the Hellings-Downs curve. Recently, pulsar timing array experiments around the world published the first evidence of nanohertz gravitational waves in the form of a gravitational wave background. In this talk, I will discuss how pulsar timing arrays detect gravitational waves, how we construct pulsar timing arrays, and describe recent results from the NANOGrav collaboration and the International Pulsar Timing Array (IPTA) collaboration.

      Relatore: Sarah Vigeland
      vigeland.pdf
    • 25
      The Hubble tension: Status and Perspectives Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)

      The success of the LCDM standard model of cosmology has now been established across a wide range of scales. Yet, despite this incredible success the precise nature of its ingredients has so far remained elusive.
      To this end, in the past decades a vast experimental effort has been undertaken to measure observables in the local and distant universe to unprecedented precision. These promising measurements have only deepened the mysteries of cosmology, however, as they revealed a growing tension between the current expansion rate of the Universe (specified by the Hubble constant) measured through the local distance ladder and that inferred from the cosmic microwave background. Now that the formal significance of this discrepancy has reached a level of five sigma significance, it is crucial to thoroughly re-examine the astrophysical observations at the heart of this Hubble tension. Similarly important is the role of looking at the future experimental efforts that are certain to bring striking new evidence that will help us to solve this cosmic puzzle.

      Relatore: Nils Schöneberg
      2024_02_14_Rome_v2.pdf
    • 10:30
      Coffee Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
    • 26
      Constraints on cosmological sources of gravitational waves with pulsar timing arrays Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
      Relatore: Gabriele Franciolini (CERN)
      Franciolini.pdf
    • 27
      Gravitational wave analysis with machine learning Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
      Relatore: Maximilian Dax
      dax_roma_02-24.pdf
    • 12:30
      Lunch Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
    • WG4: GWs & Cosmology: Overview and contributed talks Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
      Coordinatori: Carlo Tasillo (DESY Hamburg), Simone Mastrogiovanni (Istituto Nazionale di Fisica Nucleare)
      • 28
        Overview by Conveneers
        Relatori: Carlo Tasillo (DESY Hamburg), Simone Mastrogiovanni (Istituto Nazionale di Fisica Nucleare)
        WG4_overview_JENAS.pdf
      • 29
        Timing the cosmic expansion with populations of gravitational waves dark sirens
        Relatore: Simone Mastrogiovanni (Istituto Nazionale di Fisica Nucleare)
        Jenas_mastrogiovanni (1).pdf
      • 30
        A Global Network of Cavities to Search for Gravitational Waves (GravNet): A novel scheme to hunt gravitational waves signatures from the early universe
        Relatore: Kristof Schmieden (CERN)
        GravNet_Rome.pdf
    • WG4: GWs & Cosmology: WG4 Talks Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
      • 31
        Exploring new physics with pulsar timing arrays
        Relatore: Carlo Tasillo (DESY Hamburg)
        2024_02_08_PTAs_Rome_Carlo_Tasillo.pdf
      • 32
        New probe for non-Gaussianities with primordial black hole induced gravitational waves

        We propose a new probe of primordial non-Gaussianities through
        the observational window of gravitational waves (GW) being induced by
        ultra-light ($M_{\text{PBH}}< 10^{9}\rm{g}$) primordial black holes
        (PBHs). An existence of primordial non-Gaussianity can leave imprints on
        the clustering properties of PBHs and the spectral shape of the induced
        GW signal. Focusing on local-type non-Gaussianities, we find a
        distinctive double-peaked GW energy spectrum which, depending on the PBH
        mass $M$ and the initial PBH abundance at formation time, i.e.
        $\Omega_\mathrm{PBH,f}$, can lie within the frequency bands of
        forthcoming GW detectors, including LISA, ET, SKA and BBO, hence
        rendering this signal promisingly detectable by GW experiments and
        promoting it as a novel portal probing non-Gaussianities. Moreover, by
        accounting on BBN bounds on the non-Gaussian GW amplitude we set
        model-independent constraints on the effective $\tau_\mathrm{NL}$,
        denoted as $\bar{\tau}_\mathrm{NL}(k)$, on scales
        $k>10^5\mathrm{Mpc}^{-1}$, which read as $\bar{\tau}_\mathrm{NL}(k) \mathcal{P}_{\cal R}(k) < 2\times 10^{-20} \Omega^{-17/9}_\mathrm{PBH,f} \left( \frac{M_{\rm PBH}}{10^4\mathrm{g}} \right)^{-17/9}$, where
        $\mathcal{P}_{\cal R}(k)$ is the primordial curvature power spectrum.

        Relatore: Theodoros Papanikolaou
        Rome Talk.pdf
    • 16:10
      Coffee Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
    • Podium 1: Report from Conveners of WG1, WG2 Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)

      Podium Discussion
      • Input from HIC still active area of research – „known“ constraints may change in the future due to new experimental results
      • Need continuous exchange between communities
      • Input from nuclear structure and atomic physics
      • Similarly how can more interaction be encouraged?
      • General questions:
      • How can we get to a honest and realistic estimate of the systematic errors from: • EoS constraints from HIC
      • Nuclear structure calculations
      • BNSM simulations themselves
      • Is there any “new” type of input from NP or AP which can help improving the GW predictions?

      Coordinatori: Jan Steinheimer-Froschauer (Frankfurt Institute for Advanced Studies), Joachim Stroth (Goethe University Frankfurt), Massimo Mannarelli (Istituto Nazionale di Fisica Nucleare), Violetta Sagun (University of Coimbra)
    • 33
      Board Meeting Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
  • giovedì 15 febbraio
    • GW detectors at all frequencies: various contributions Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
      • 34
        The challenge of Low Frequency sensitivity enhancement with Einstein Telescope, a general overview
        Relatore: Ettore Majorana (Istituto Nazionale di Fisica Nucleare)
        BU_ET_Majorana.pdf
      • 35
        LISA, the first space-based gravitational wave observatory
        Relatore: Alberto Sesana (Universita` di Milano Bicocca)
        Sesana_Rome24.pdf
      • 36
        Closing gaps in the GW spectrum: new physics with muHz GWs and ideas to detect them
        Relatore: Diego Blas Temiño
        02Rome.pdf
      • 37
        Opportunities for gravitational wave searches at high frequencies
        Relatore: Krisztian Peters
        hfgw_jenas.pdf
      • 38
        Round Table
    • 11:00
      Coffee Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
    • 39
      GW tests of gravity: past, present and future Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
      Relatore: Michalis Agathos
    • 40
      Distinguishing between environmental effects around binary black holes Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
      Relatore: Philippa Cole (University of Amsterdam)
      Cole_Rome_2024.pdf
    • 13:00
      Lunch Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
    • WG3: Fundamental problems in high-energy and gravitational physic: GWs and Dark Matter Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
      Coordinatori: Cristiano Palomba (Istituto Nazionale di Fisica Nucleare), Philippa Cole (University of Amsterdam), Richard Brito
      • 41
        Dynamical friction on compact binary systems
        Relatore: Vincent Desjacques
        CompactBDF.pdf
    • Podium 2: Report from Conveners of WG3 and WG4 Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
      Coordinatori: Carlo Tasillo (DESY Hamburg), David Keitel (UIB), Elisa Maggio (Max Planck Institute for Gravitational Physics, Albert Einstein Institute, Potsdam), Simone Mastrogiovanni (Istituto Nazionale di Fisica Nucleare)
      WG3_WG4_podium_Jenas.pdf
    • 16:25
      Coffee Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
  • venerdì 16 febbraio
    • 42
      Primordial Black Holes: formation and cosmological impact in the current Universe Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
      Relatore: Dr. Ilia Musco (Istituto Nazionale di Fisica Nucleare, Rome)
      Musco_Jenas24.pdf
    • 43
      A Bayesian investigation of the neutron star equation-of-state vs. gravity degeneracy Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
      Relatore: Bhaskar Biswas (Universität Hamburg)
    • 44
      Some aspects of the three-body problem in General Relativity Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
      Relatore: Adrien Benoit Kuntz (SISSA, Trieste)
    • 45
      Closing and Next Actions Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
      Relatori: Paolo Pani (Sapienza University of Rome & INFN Roma1), Tetyana Galatyuk (TU Darmstadt / GSI)
    • 10:55
      Coffee Physics Department - Aula Amaldi (Marconi Building)

      Physics Department - Aula Amaldi (Marconi Building)

      Sapienza University of Rome

      Piazzale Aldo Moro, 5 · 06 49911 Rome (Italy)
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