NEUMATT

NEUtron star MATTer

 

 

SELECTED PUBLICATIONS

 
INFN Sezione di Catania
  1. Convergence of the Hole-Line Expansion with Modern Nucleon-Nucleon Potentials  J.J. Lu, Z.H. Li, C.Y. Chen, M. Baldo, H.-J. Schulze. Phys. Rev. C 96, 044309 (2017).
  2. Hyperons: The Strange Ingredients of the Nuclear Equation of State. I. Vidaña. Proc. R. Soc. A 474: 20180145 (2018).
  3. Nuclear Equation of State for Compact Stars and Supernovae. G.F. Burgio, A. Fantina. The Physics and Astrophysics of Neutron Stars (Astrophysics and Space Science Library Book 457), Springer (2018).
  4. Neutron Star Cooling with Microscopic Equations of State. J.B. Wei, G.F. Burgio, H.-J. Schulze. MNRAS 484, 5162 (2019).
  5. On the Change of Old Neutron Star Masses with Galactocentric Distance. A. Del Popolo, M. Deliyergiyev, M. Le Delliou, L. Tolos, G.F. Burgio. Physics of the Dark Universe 28, 100484 (2020).

 

INFN Sezione di Ferrara
  1. The scenario of two families of compact stars. A. Drago, G. Pagliara, A. Lavagno, D. Pigato. Eur.Phys.J.A 52 (2016) 2, 40 and 41.
  2. Convective Excitation of Inertial Modes in Binary Neutron Star Mergers. R. De Pietri, A. Feo, J.A. Font, F. Loeffler, F. Maione, M. Pasquali, N. Stergioulas. Phys. Rev. Lett. 120 (2018) 221101
  3. Merger of two neutron stars: predictions from the two-families scenario. A. Drago, G. Pagliara. Astrophys.J.Lett. 852 (2018) 2, L32.
  4. Are Small Radii of Compact Stars Ruled out by GW170817/AT2017gfo? F. Burgio, A. Drago, G. Pagliara, H.-J. Schulze, J.-B. Wei. Astrophys.J. 860 (2018) 2, 139.
  5. Merger of compact stars in the two-families scenario. R. De Pietri, A. Drago, A. Feo, G. Pagliara, M. Pasquali, S. Traversi, and G. Wiktorowicz. Astrophys.J. 881 (2019) 2, 122.

 

INFN-LNGS
  1. Torsional oscillations of nonbare strange stars. M.Mannarelli, G.Pagliaroli, A.Parisi, L.Pilo and F.Tonelli. Astrophys. J. 815 (2015) no.2, 81
  2. Measuring the neutron star compactness and binding energy with supernova neutrinos. A. Gallo Rosso, F. Vissani and M.C.Volpe. JCAP 11(2017), 036
  3. Pinpointing astrophysical bursts of low-energy neutrinos embedded into the noise. C.Casentini, G.Pagliaroli, C.Vigorito and V.Fafone. JCAP 08 (2018), 010
  4. Gravitational wave echoes from strange stars. M.Mannarelli and F.Tonelli. Phys. Rev. D 97 (2018) 123010
  5. Meson condensation. M.Mannarelli. Particles 2 (2019) no.3, 411

 

INFN Sezione di Milano
  1. Constraints on pulsar masses from the maximum observed glitch. P. M. Pizzochero, M. Antonelli, B. Haskell and S. Seveso. Nature Astronomy 1 (2017) 0134.
  2. Effects of general relativity on glitch amplitudes and pulsar mass upper bounds. M. Antonelli, A. Montoli and P. M. Pizzochero, Monthly Notices of the Royal Astronomical Society 475 (2018) 5
  3. The role of mass, equation of state and superfluid reservoir in large pulsar glitches. A. Montoli, M. Antonelli and P. M. Pizzochero. Monthly Notices of the Royal Astronomical Society 492 (2020) 4837
  4. Core and crust contributions in overshooting glitches: the Vela pulsar 2016 glitch. P. M. Pizzochero, A. Montoli and M. Antonelli. Astronomy&Astrophysics 636 (2020) A101.
  5. A universal formula for the relativistic correction to the mutual friction coupling time-scale in neutron stars. L. Gavassino, M. Antonelli, P. M. Pizzochero and B. Haskell. Monthly Notices of the Royal Astronomical Society 494 (2020) 3562.

 

INFN Sezione di Pisa
  1. Two Coexisting Families of Compact Stars: Observational Implications for Millisecond Pulsars. S. Bhattacharyya, I. Bombaci, D. Logoteta, A.V .Thampan. Astrophys. Jour.  848 (2017) 65.
  2. Equation of state of dense nuclear matter and neutron star structure from nuclear chiral interactions. I. Bombaci, D. Logoteta. Astron. and Astrophys. 609 (2018) A128.  
  3.  Effects of chiral effective field theory equation of state on binary neutron star mergers. A. Endrizzi, D. Logoteta, B. Giacomazzo, I. Bombaci, W. Kastaun, R. Ciolfi. Phys. Rev. D 98 (2018) 043015. 
  4. Impact of chiral hyperonic three-body forces on neutron stars. D. Logoteta, I. Vidana, I. Bombaci. European Physical Journal A 55 (2019) 207.
  5.  Benchmark calculations of pure neutron matter with realistic nucleon-nucleon interactions. M. Piarulli, I. Bombaci, D. Logoteta, A. Lovato, R. B. Wiringa. Physical Review C 101 (2020) 045801
 
 
 

NEUMATT

NEUtron star MATTer

 



JOB OPPORTUNITY

Postdoc position in the Neutron Star Matter theory group at the Pisa INFN Section: Modelling the equation of state of dense and hot matter for astrophysical applications.

The Neutron Star Matter (NEUMATT) theory group at the Pisa INFN Section has an opening for a 2-year postdoc position in the field of Extreme Matter and Compact Object Physics sponsored by the National Institute for Nuclear Physics (INFN) Job opportunuty N. 25864. The postdoc will work at the Pisa INFN Section and Physics Department of the University of Pisa in collaboration with Prof. Ignazio Bombaci. The research topic is “Modelling the equation of state of dense and hot matter for astrophysical applications”.

The deadline for applications is November 10 2023 (11:59 a.m. CET). Applications are only accepted online via the following link: https://reclutamento.dsi.infn.it/ Bando N. 25864 (job number 25864).

In the application the candidate will be requested to indicate the INFN Section (Sezione di Pisa) and the research topic (Modelling the equation of state of dense and hot matter for astrophysical applications) since the call N. 25864 includes other 14 topics in different INFN Sections. Full instructions in English can be found on the file “Pdf Bando” Job opportunuty N. 25864

The research topics of the Pisa NEUMATT group have focused mainly on the following aspects of theoretical nuclear physics and relativistic asctrophysics: Nuclear quantum many-body problem; Equation of state of hadronic matter under extreme conditions; Quark deconfinement phase transition in dense matter and related astrophysical phenomena; Numerical General Relativity: Neutron star structure and evolution, Binary neutron stars merging and related astrophysical phenomena.

More recently the research activity has focused on the study of newborn neutron stars and postmerger compact objects.

Beside the thermal effects already included in our recent calculations of the EoS of nuclear matter, we also started to investigate the role of neutrino trapping on the EoS and thus to study the structure and early evolution of newborn neutron stars. In particular we started to investigate in addition to static (i.e. non-rotating) configurations also rapidly rotating stars assuming rigid or differential rotation. This study is extremely relevant to investigate the evolution of a newly born neutron star, the concept of neutron star limiting mass and the fate of the postmerger compact object formed in a BNS merger.

 

   Some recent publications

[1]    D. Logoteta, A. Perego, I Bombaci, Microscopic equation of state of hot nuclear matter for numerical relativity simulations, Astronomy and Astrophysics 646 (2021) A55.

 

[2]   D. Logoteta, Hyperons in Neutron Stars, Universe 7 (11) (2021) 408.

 

[3] A. Prakash, D. Radice, D. Logoteta, A. Perego, V. Nedora, I. Bombaci, R. Kashyap, S. Bernuzzi, A. Endrizzi, Andrea, Signatures of deconfined quark phases in binary neutron star mergers, Physical Review D 104 (2021) 083029.

 

[4]   I. Bombaci, A. Drago, D. Logoteta, G. Pagliara, I. Vidaña, Was GW190814 a Black Hole-Strange Quark Star System?, Physical Review Letters, 126 (2021) 162702.

 

[5]   D. Logoteta, I. Bombaci, A. Perego, Isoentropic equations of state of beta-stable hadronic matter with a quark phase transition, EPJ A 58 (2022) 55.

 

[6]   I. Bombaci, The Hyperon Puzzle in Neutron Stars, Nuclear Physics News, 31:3, (2021) 17-21, DOI: 10.1080/10619127.2021.1915024 

 

[7] I. Bombaci, The Equation of State of Neutron Star Matter, Chap.9 in the book Millisecond Pulsars, Astrophysics and Space Science Library (ASSL, volume 465) Springer Nature Switzerland (2022)

[8] A. Lovato, I. Bombaci, D. Logoteta, M. Piarulli, R. B. Wiringa, Benchmark calculations of infinite neutron matter with realistic two- and three-nucleon potentials, Phys. Rev. C 105 (2022) 055808.

[9] R. Kashyap, A. Das, D. Radice, S. Padamata, A. Prakash, D. Logoteta, A. Perego, D. A. Godzieba, S. Bernuzzi, I. Bombaci, F. J. Fattoyev, B. T. Reed, A. D. Schneider, Numerical relativity simulations of prompt collapse mergers: Threshold mass and phenomenological constraints on neutron star properties after GW170817, Phys. Rev. D 105 (2022) 103022.

[10] I. Vidana, D. Logoteta, I. Bombaci, Effect of chiral nuclear forces on the neutrino mean free path in hot neutron matter, Physical Review C 106 (2022) 035804

 

Pisa, world-famous for its leaning tower and for having been the birthplace of Galileo Galilei, is a beautiful small city in Tuscany close to the sea and with an international airport just a few kilometers from the city center. The gravitational wave interferometer VIRGO is located in the Pisa countryside, and research on gravitational waves is a major experimental activity at the Pisa INFN Section and at the Physics Department of the University of Pisa.

For inquire please do not hesitate to contact Prof. Ignazio Bombaci (This email address is being protected from spambots. You need JavaScript enabled to view it.)

 

 
 
 
 

QUAGRAP

The interface of gravity and quantum mechanics

 

 

Scientific activities of the various Research Units


 

 Albeit sharing common objectives the three knots of the network (Cagliari, Napoli and Trieste) have over time diversified their lines of research, which in this sense can be taken as complementary.

Cagliari Unit: This unit is based in Cagliari University (with the participation of Prof. Di Salvo from Palermo University). The members are experts in gravitational theories and in astrophysics. The planned research will concern noncommutative quantum field theory, with special attention to possible experimentally verifiable implications, like breaking of discrete symmetries or DSR-related effects. Another topic of research will be the possibility that long-range quantum gravity effects could play a role at galactic scales and could be responsible for effects usually ascribed to dark matter. Finally, we plan to investigate the possible signatures of the near-horizon geometry of black holes and other quantum gravity effects deducible from the observation of the properties of gravitational waves generated by the merging of black holes. The presence of astrophysicists in the group warrants a specific attention to the observational side.

Napoli Unit: This unit is based at Federico II University of Naples. The main lines of research planned for the near future are both on the more formal/mathematical aspects of the QG problem and in quantum-gravity phenomenology. On the formal side, we plan to focus on reaching a deeper understanding of the noncommutative spacetimes which are potentially relevant for the quantum-gravity problem, including the Snyder spacetime and the kappa-Minkowski spacetime. A large international effort over the last decade (with key contributions by members of our group) has allowed a solid understanding of classical field theories in these spacetimes, but several hurdles must be faced in order to reach the much-needed formulation of the associated quantum field theories. On the phenomenology side, we shall focus mainly on the opportunities which are expected to arise through the use of novel multisatellite telescopes and by the advent of multimessenger astronomy. Amelino-Camelia leads one of the working groups of the HERMES collaboration which is planning to deploy such a multi-satellite telescope, particularly suited for searching for traces of quantum spacetime-induced anomalous propagation of photons coming from distant gamma-ray sources. Moreover, the Napoli unit is involved in similar searches involving astrophysical neutrinos produced in gamma-ray bursts.

Trieste Unit: this is based in SISSA (with the participation of Prof. R. Balbinot from University of Bologna) and has a long-standing tradition in gravitation theory. The main lines of research planned for the near future are both on the theoretical side as well as on the experimental one. On the theoretical side the TS group will focus on the development and extension of theoretical frameworks, from DSR, SME, non-local/non-commutative effective field theory (EFT) and modified dispersion relations, to quantum-gravity-induced black hole mimickers and Finsler geometries, aiming at describing possible scenarios for low energy (sub-Planckian) effects induced by quantum gravity theories. In doing so it will also further exploit Analogue Models of gravity as toy models of emergent spacetime. On the experimental side we plan to have a close interaction with observational multi-messenger astrophysics (in particular for possible signature of deviations from standard black hole physics in gravitational wave events) and experiments in quantum optics and atomic physics aimed at testing several quantum aspects of gravitation.

 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 

QUAGRAP

The interface of gravity and quantum mechanics

 

 

Abstract


  1. The search for a quantum gravity theory has been for a long time the subject of intense research. While we have nowadays several competing frameworks, none of them can yet claim to be a complete, fully predictive, theory. Even worse, the lack of experimental guidance has so far limited our options for selecting one proposal over the others. Quantum gravity phenomenology is an operational framework based on the realization that new physical phenomena, associated to some quantum gravity scenarios, can be amenable to observational/experimental tests even without directly accessing the Planck scale. The study of such theoretical possibilities, and of their phenomenological implications, is a typically interdisciplinary activity requiring the exchange of ideas between theoretical, experimental and observational communities. This research project aims at being a catalyst for research in quantum gravity phenomenology at the national and international level, by aggregating the core of Italian researchers in this field and at the same time be pivotal in creating an interdisciplinary network of collaborations within INFN and outside of it. The research activity is aimed at developing theoretical frameworks, including quantum spacetime models entailing departures from Lorentz symmetries and analogue gravity models, as well as exploiting at its best the wealth of data (available and expected) from multi-messenger astrophysics observations and high precision experiments.

 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 
 

QUAGRAP

The interface of gravity and quantum mechanics

 

 

National Coordinator:  Stefano Liberati, SISSA, Trieste

 

INFN Unit Cagliari
Staff members

Prof. Salvatore Mignemi (PO, UniCagliari, 100%)

Prof. Mariano Cadoni (PO, UniCagliari, 60%)

Prof. Luciano Burderi (PA, UniCagliari, 90%)

Prof. Tiziana Di Salvo (PO, UniPalermo, 100%)

Dr. Andrea Sanna (RTDb, UniCagliari, 100%)

Other participants (Post-docs, Ph.D students,...)

Dr. Piero Olla (Ricercatore CNR 50%)

Mauro Oi, PhD student 3rd year (100%)

Zakaria Belkhadia, PhD student 3rd year (100%)

 

INFN Unit Napoli
Staff members

Prof. Giovanni Amelino-Camelia (PO, 100%)

Dr. Michele Arzano (RTDB, Uni. Napoli, 100%)

Dr. Giulia Gubitosi (RTDA, Uni. Napoli, 100%)

Other participants (Post-docs, Ph.D students,...)

Vittorio D’Esposito, PhD student 3rd year  (100%)

Pietro Pellecchia, PhD student 1st year (100%)

 

INFN Unit Trieste
Staff members

Prof. Stefano Liberati (PO, SISSA, 100%)

Prof. Roberto Balbinot (PA, Uni. Bologna. 100%)

Prof. Marco Bruni (PA University of Portsmouth, 50%)

Other participants (Post-docs, Ph.D students,...)

Dr.Marc Schneider,postdoc 

Vania Vellucci, PhD student 3rd year (100%)

Francesco Del Porro, PhD student 3rd year (100%)

Giulio Neri, PhD student 2nd year (100%)

 
 
 
 
 
 
 
 

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