| Constraints on pulsar masses from the maximum observed glitch PM Pizzochero, M Antonelli, B Haskell, S Seveso Nature Astronomy 1 (7), 0134, 2017 | 59 | 2017 |
| Thermodynamic stability implies causality L Gavassino, M Antonelli, B Haskell Physical Review Letters 128 (1), 010606, 2022 | 51 | 2022 |
| When the entropy has no maximum: A new perspective on the instability of the first-order theories of dissipation L Gavassino, M Antonelli, B Haskell Physical Review D 102 (4), 043018, 2020 | 43 | 2020 |
| Bulk viscosity in relativistic fluids: from thermodynamics to hydrodynamics L Gavassino, M Antonelli, B Haskell Classical and Quantum Gravity 38 (7), 075001, 2021 | 40 | 2021 |
| Crust or core? Insights from the slow rise of large glitches in the Crab pulsar B Haskell, V Khomenko, M Antonelli, D Antonopoulou Monthly Notices of the Royal Astronomical Society: Letters 481 (1), L146-L150, 2018 | 36* | 2018 |
| Thermodynamics of uncharged relativistic multifluids L Gavassino, M Antonelli Classical and Quantum Gravity 37 (2), 025014, 2019 | 33 | 2019 |
| Unified Extended Irreversible Thermodynamics and the stability of relativistic theories for dissipation L Gavassino, M Antonelli Frontiers in Astronomy and Space Sciences 8, 686344, 2021 | 28* | 2021 |
| A universal formula for the relativistic correction to the mutual friction coupling time-scale in neutron stars L Gavassino, M Antonelli, PM Pizzochero, B Haskell Monthly Notices of the Royal Astronomical Society 494 (3), 3562-3580, 2020 | 26 | 2020 |
| Core and crust contributions in overshooting glitches: the Vela pulsar 2016 glitch PM Pizzochero, A Montoli, M Antonelli Astronomy & Astrophysics 636, A101, 2020 | 26 | 2020 |
| Superfluid vortex-mediated mutual friction in non-homogeneous neutron star interiors M Antonelli, B Haskell Monthly Notices of the Royal Astronomical Society 499 (3), 3690-3705, 2020 | 25 | 2020 |
| Axially symmetric equations for differential pulsar rotation with superfluid entrainment M Antonelli, PM Pizzochero Monthly Notices of the Royal Astronomical Society 464 (1), 721-733, 2017 | 25 | 2017 |
| Bayesian estimate of the superfluid moments of inertia from the 2016 glitch in the Vela pulsar A Montoli, M Antonelli, F Magistrelli, PM Pizzochero Astronomy & Astrophysics 642, A223, 2020 | 24 | 2020 |
| Effects of general relativity on glitch amplitudes and pulsar mass upper bounds M Antonelli, A Montoli, PM Pizzochero Monthly Notices of the Royal Astronomical Society 475 (4), 5403-5416, 2018 | 23 | 2018 |
| Multifluid modelling of relativistic radiation hydrodynamics L Gavassino, M Antonelli, B Haskell Symmetry 12 (9), 1543, 2020 | 21 | 2020 |
| Symmetric-hyperbolic quasihydrodynamics L Gavassino, M Antonelli, B Haskell Physical Review D 106 (5), 056010, 2022 | 19 | 2022 |
| The role of mass, equation of state, and superfluid reservoir in large pulsar glitches A Montoli, M Antonelli, PM Pizzochero Monthly Notices of the Royal Astronomical Society 492 (4), 4837-4846, 2020 | 19 | 2020 |
| Modelling strains and stresses in continuously stratified rotating neutron stars E Giliberti, G Cambiotti, M Antonelli, PM Pizzochero Monthly Notices of the Royal Astronomical Society 491 (1), 1064-1078, 2020 | 18 | 2020 |
| Simulating bulk viscosity in neutron stars. I. Formalism G Camelio, L Gavassino, M Antonelli, S Bernuzzi, B Haskell Physical Review D 107 (10), 103031, 2023 | 16 | 2023 |
| Extending Israel and Stewart hydrodynamics to relativistic superfluids via Carter’s multifluid approach L Gavassino, M Antonelli, B Haskell Physical Review D 105 (4), 045011, 2022 | 15 | 2022 |
| The effect of non-linear mutual friction on pulsar glitch sizes and rise times T Celora, V Khomenko, M Antonelli, B Haskell Monthly Notices of the Royal Astronomical Society 496 (4), 5564-5574, 2020 | 14 | 2020 |
Pierre M. PizzocheroUniversità degli Studi di MilanoBestätigte E-Mail-Adresse bei unimi.it
