Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects | Paper Citation Record

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This paper cites We show in Fig.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects We show in Fig

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This paper cites After the core bounce, the shock wave stalls and recedes as a result of intense mass accretion.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects After the core bounce, the shock wave stalls and recedes as a result of intense mass accretion

Reference 2

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Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Unresolved cited work

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This paper cites Equations of state for supernovae and compact stars.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Equations of state for supernovae and compact stars

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This paper cites Equation of state in neutron stars and supernovae.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Equation of state in neutron stars and supernovae

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This paper cites Multiple physical elements to determine the gravitational-wave signatures of core-collapse supernovae.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Multiple physical elements to determine the gravitational-wave signatures of core-collapse supernovae

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This paper cites Physics of Core-Collapse Supernovae in Three Dimensions: a Sneak Preview.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Physics of Core-Collapse Supernovae in Three Dimensions: a Sneak Preview

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Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Explosion Mechanisms of Core-Collapse Supernovae

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This paper cites Perspectives on Core-Collapse Supernova Theory.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Perspectives on Core-Collapse Supernova Theory

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Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Unresolved cited work

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This paper cites Janka, Neutrino-Driven Explosions, inHandbook of Supernovae, ISBN 978-3-319-21845-.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Janka, Neutrino-Driven Explosions, inHandbook of Supernovae, ISBN 978-3-319-21845-

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This paper cites 1095(Springer, 2017) p.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects 1095(Springer, 2017) p

Reference 14

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Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Unresolved cited work

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This paper cites Dynamics and Equation of State Dependencies of Relevance for Nucleosynthesis in Supernovae and Neutron Star Mergers.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Dynamics and Equation of State Dependencies of Relevance for Nucleosynthesis in Supernovae and Neutron Star Mergers

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This paper cites Neutrino Emission as Diagnostics of Core-Collapse Supernovae.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Neutrino Emission as Diagnostics of Core-Collapse Supernovae

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Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Neutron Stars and the Nuclear Equation of State

Reference 18

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This paper cites Chatziioannou, H.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Chatziioannou, H

Reference 19

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Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Kotake, K

Reference 20

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This paper cites Supernova Neutrinos: Production, Oscillations and Detection.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Supernova Neutrinos: Production, Oscillations and Detection

Reference 21

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This paper cites Takahara and K.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Takahara and K

Reference 22

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This paper cites Gravitational Waves from Core-Collapse Supernovae.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Gravitational Waves from Core-Collapse Supernovae

Reference 23

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This paper cites Core-Collapse Supernovae and their Gravitational Wave Signals: The Status of Theory and Modeling.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Core-Collapse Supernovae and their Gravitational Wave Signals: The Status of Theory and Modeling

Reference 24

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This paper cites Sotani, Understanding supernova gravitational waves with protoneutron star asteroseis- mology, Classical and Quantum Gravity43, 093001 (2026).

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Sotani, Understanding supernova gravitational waves with protoneutron star asteroseis- mology, Classical and Quantum Gravity43, 093001 (2026)

Reference 25

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This paper cites Baron, J.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Baron, J

Reference 26

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Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Core-collapse supernova equations of state based on neutron star observations

Reference 27

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Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Unresolved cited work

Reference 28

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This paper cites Shock Breakout in Core-Collapse Supernovae and its Neutrino Signature.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Shock Breakout in Core-Collapse Supernovae and its Neutrino Signature

Reference 29

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This paper cites Postbounce evolution of core-collapse supernovae: Long-term effects of equation of state.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Postbounce evolution of core-collapse supernovae: Long-term effects of equation of state

Reference 30

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This paper cites Core-collapse supernova explosions triggered by a quark-hadron phase transition during the early post-bounce phase.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Core-collapse supernova explosions triggered by a quark-hadron phase transition during the early post-bounce phase

Reference 31

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This paper cites Equation of State Effects on Gravitational Waves from Rotating Core Collapse.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Equation of State Effects on Gravitational Waves from Rotating Core Collapse

Reference 32

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Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Equation-of-State Dependent Features in Shock-Oscillation Modulated Neutrino and Gravitational-Wave Signals from Supernovae

Reference 33

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This paper cites On the Importance of the Equation of State for the Neutrino-Driven Supernova Explosion Mechanism.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects On the Importance of the Equation of State for the Neutrino-Driven Supernova Explosion Mechanism

Reference 34

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Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects The Dependence of the Neutrino Mechanism of Core-Collapse Supernovae on the Equation of State

Reference 35

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Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Symmetry energy impact in simulations of core-collapse supernovae

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This paper cites Equation of State Dependence of Gravitational Waves in Core-Collapse Supernovae.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Equation of State Dependence of Gravitational Waves in Core-Collapse Supernovae

Reference 37

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This paper cites Crucial Physical Dependencies of the Core-Collapse Supernova Mechanism.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Crucial Physical Dependencies of the Core-Collapse Supernova Mechanism

Reference 38

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This paper cites Simulations of core-collapse supernovae in spatial axisymmetry with full Boltzmann neutrino transport.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Simulations of core-collapse supernovae in spatial axisymmetry with full Boltzmann neutrino transport

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This paper cites On the Neutrino Distributions in Phase Space for the Rotating Core-collapse Supernova Simulated with a Boltzmann-neutrino-radiation-hydrodynamics Code.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects On the Neutrino Distributions in Phase Space for the Rotating Core-collapse Supernova Simulated with a Boltzmann-neutrino-radiation-hydrodynamics Code

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This paper cites Equation of state effects in the core collapse of a $20$-$M_\odot$ star.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Equation of state effects in the core collapse of a $20$-$M_\odot$ star

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This paper cites Dynamics and neutrino signal of black hole formation in non-rotating failed supernovae. I. EOS dependence.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Dynamics and neutrino signal of black hole formation in non-rotating failed supernovae. I. EOS dependence

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Observation a4d82a53-0c11-4efd-9d51-c765a53f33fa · outbound

This paper cites Effect of the Nuclear Equation of State on Relativistic-Turbulence Induced Core-Collapse Supernovae.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Effect of the Nuclear Equation of State on Relativistic-Turbulence Induced Core-Collapse Supernovae

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Resolution: verified exact; local_arxiv, observed 2026-08-08T10:10:49.440379Z

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This paper cites Impact of the nuclear equation of state on the explodability of massive stars.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Impact of the nuclear equation of state on the explodability of massive stars

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This paper cites An Exploration of the Equation of State Dependence of Core-Collapse Supernova Explosion Outcomes and Signatures.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects An Exploration of the Equation of State Dependence of Core-Collapse Supernova Explosion Outcomes and Signatures

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This paper cites Neutrino signals from the formation of black hole: a probe of equation of state of dense matter.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Neutrino signals from the formation of black hole: a probe of equation of state of dense matter

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Resolution: verified exact; local_arxiv, observed 2026-08-08T10:10:49.383558Z

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This paper cites Black Hole Supernovae, their Equation of State Dependence and Ejecta Composition.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Black Hole Supernovae, their Equation of State Dependence and Ejecta Composition

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This paper cites Black Hole Formation in Failing Core-Collapse Supernovae.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Black Hole Formation in Failing Core-Collapse Supernovae

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This paper cites A Comparative study of hyperon equations of state in supernova simulations.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects A Comparative study of hyperon equations of state in supernova simulations

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This paper cites Equation of State Dependent Dynamics and Multimessenger Signals from Stellar-mass Black Hole Formation.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Equation of State Dependent Dynamics and Multimessenger Signals from Stellar-mass Black Hole Formation

Reference 50

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This paper cites Equation of State and Progenitor Dependence of Stellar-Mass Black-Hole Formation.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Equation of State and Progenitor Dependence of Stellar-Mass Black-Hole Formation

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Observation 0f78a5ee-1f4e-474e-9f84-bb0b752751b8 · outbound

This paper cites Suzuki, inPhysics and Astrophysics of Neutrinos, edited by M.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Suzuki, inPhysics and Astrophysics of Neutrinos, edited by M

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Resolution: verified fuzzy; raw_fallback, observed 2026-08-08T10:10:50.490199Z

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Observation 714a6978-9349-4ec1-b31e-1f8bd8a4d395 · outbound

This paper cites Yasin, S.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Yasin, S

Reference 53

Resolution: verified fuzzy; raw_fallback, observed 2026-08-08T10:10:50.524049Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 67468d6e-2422-4d0c-94b3-4708d0dce7b4 · outbound

This paper cites The APR equation of state for simulations of supernovae, neutron stars and binary mergers.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects The APR equation of state for simulations of supernovae, neutron stars and binary mergers

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-08T10:10:48.394357Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e8171e5f-39e4-4cb3-a375-cf5935379b9c · outbound

This paper cites Influence of the effective mass on the properties of nuclear matter at finite density and temperature.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Influence of the effective mass on the properties of nuclear matter at finite density and temperature

Reference 55

Resolution: verified exact; local_arxiv, observed 2026-08-08T10:10:49.220576Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 388ca1a0-dd90-4225-923e-32f6372e1730 · outbound

This paper cites Burrows and J.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Burrows and J

Reference 56

Resolution: verified fuzzy; raw_fallback, observed 2026-08-08T10:10:50.505621Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 859fb60d-e572-4906-a0a2-da85b3a3defa · outbound

This paper cites Cooling timescale for protoneutron stars and properties of nuclear matter: Effective mass and symmetry energy at high densities.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Cooling timescale for protoneutron stars and properties of nuclear matter: Effective mass and symmetry energy at high densities

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-08T10:10:48.432957Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4a3d64b1-4fac-4af3-813c-752a080443d5 · outbound

This paper cites Influence of the symmetry energy on the birth of neutron stars and supernova neutrinos.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Influence of the symmetry energy on the birth of neutron stars and supernova neutrinos

Reference 58

Resolution: verified exact; local_arxiv, observed 2026-08-08T10:10:49.196300Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation fdf88342-7a89-45a1-a412-cb85fd52011a · outbound

This paper cites Evolution of Protoneutron Stars.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Evolution of Protoneutron Stars

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-08T10:10:48.418288Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ebff9801-c6aa-4aac-823f-713c0032a254 · outbound

This paper cites Proto-Neutron Star Cooling with Convection: The Effect of the Symmetry Energy.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Proto-Neutron Star Cooling with Convection: The Effect of the Symmetry Energy

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-08T10:10:48.423272Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c41d4d0a-8fe2-407e-a926-8a7147727498 · outbound

This paper cites Supernova Neutrino Light Curves and Spectra for Various Progenitor Stars: From Core Collapse to Proto-neutron Star Cooling.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Supernova Neutrino Light Curves and Spectra for Various Progenitor Stars: From Core Collapse to Proto-neutron Star Cooling

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-08T10:10:48.428124Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1370749a-7e78-4e45-b66d-c66179833d06 · outbound

This paper cites an unresolved cited work.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Unresolved cited work

Reference 62

Resolution: verified exact; raw_fallback, observed 2026-08-08T10:10:48.938612Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 191392c5-bab0-42f7-9eb7-ee8cbb5288f8 · outbound

This paper cites Influence of effective nucleon mass on equation of state for supernova simulations and neutron stars.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Influence of effective nucleon mass on equation of state for supernova simulations and neutron stars

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-08T10:10:48.437906Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 76e79414-a315-489d-911f-217378c6d340 · outbound

This paper cites Effects of symmetry energy on equation of state for simulations of core-collapse supernovae and neutron-star mergers.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Effects of symmetry energy on equation of state for simulations of core-collapse supernovae and neutron-star mergers

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-08T10:10:48.443532Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f461c043-4b02-48c1-9d25-2db0235f25d4 · outbound

This paper cites Relativistic Equation of State for Core-Collapse Supernova Simulations.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Relativistic Equation of State for Core-Collapse Supernova Simulations

Reference 65

Resolution: verified exact; local_arxiv, observed 2026-08-08T10:10:49.080174Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 3f5c7886-6e95-4b00-a7be-325ce4ab3cf5 · outbound

This paper cites nucleons, electrons, positrons, and photons by adding the lepton and photon contributions to the nuclear contributions for pressure, energy, and entropy.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects nucleons, electrons, positrons, and photons by adding the lepton and photon contributions to the nuclear contributions for pressure, energy, and entropy

Reference 66

Resolution: verified fuzzy; raw_fallback, observed 2026-08-08T10:10:50.705197Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation ecf67bf3-95ef-4eee-818b-40e131aa6c0b · outbound

This paper cites an unresolved cited work.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Unresolved cited work

Reference 67

Resolution: verified exact; raw_fallback, observed 2026-08-08T10:10:49.057496Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation c30b2efd-e21a-4817-935c-db35dc9c83c5 · outbound

This paper cites Influence of density dependence of symmetry energy in hot and dense matter for supernova simulations.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Influence of density dependence of symmetry energy in hot and dense matter for supernova simulations

Reference 68

Resolution: verified exact; local_arxiv, observed 2026-08-08T10:10:48.707064Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 04a37a0d-1d4e-4349-a589-361c2035998a · outbound

This paper cites Sugahara and H.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Sugahara and H

Reference 69

Resolution: verified fuzzy; raw_fallback, observed 2026-08-08T10:10:50.474729Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation a91b7ff0-e7d6-4b2f-976a-2abe64a9a25f · outbound

This paper cites GW170817: Measurements of Neutron Star Radii and Equation of State.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects GW170817: Measurements of Neutron Star Radii and Equation of State

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-08T10:10:48.473746Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2d798ac9-d8d6-4736-a088-ddfee0553eb6 · outbound

This paper cites A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-08T10:10:48.478358Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fa7a60b1-add7-4195-a4a5-286193a4ed65 · outbound

This paper cites A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects A NICER View of the Massive Pulsar PSR J0740+6620 Informed by Radio Timing and XMM-Newton Spectroscopy

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-08T10:10:48.482877Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c7596981-f8d3-408d-b2ef-f1f1cd5a2599 · outbound

This paper cites an unresolved cited work.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Unresolved cited work

Reference 73

Resolution: unresolved; raw_fallback, observed 2026-08-08T10:10:50.458903Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 19b6a12d-28b3-4e76-9d21-80d5007a0422 · outbound

This paper cites an unresolved cited work.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Unresolved cited work

Reference 74

Resolution: unresolved; raw_fallback, observed 2026-08-08T10:10:50.443336Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation 46c87fa7-d0c6-4d45-b378-1ca46f69e852 · outbound

This paper cites Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Core-Collapse Supernovae from 9 to 120 Solar Masses Based on Neutrino-powered Explosions

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-08T10:10:48.496159Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a12831f2-1989-4d92-aa4c-73b6a4f951d0 · outbound

This paper cites Effects of nuclear matter and composition in core-collapse supernovae and long-term proto-neutron star cooling.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Effects of nuclear matter and composition in core-collapse supernovae and long-term proto-neutron star cooling

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-08T10:10:48.501202Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fa019ef9-5427-441d-97d6-647d5ec7a3d0 · outbound

This paper cites Heavy Nuclei as Thermal Insulation for Proto-Neutron Stars.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Heavy Nuclei as Thermal Insulation for Proto-Neutron Stars

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-08T10:10:48.506143Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation aa45121a-3a4e-4592-b070-caf1aa670735 · outbound

This paper cites A New Approach to Mass and Radius of Neutron Stars with Supernova Neutrinos.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects A New Approach to Mass and Radius of Neutron Stars with Supernova Neutrinos

Reference 78

Resolution: verified exact; local_arxiv, observed 2026-08-08T10:10:48.587029Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

Observation b51bed67-4ab0-4bfe-910a-5bb994b1dbc2 · outbound

This paper cites Observing Supernova Neutrino Light Curves with Super-Kamiokande. II. Impact of the Nuclear Equation of State.

Influence of effective mass of the relativistic mean field theory on core collapse supernovae and compact objects Observing Supernova Neutrino Light Curves with Super-Kamiokande. II. Impact of the Nuclear Equation of State

Reference 79

Resolution: verified exact; local_arxiv, observed 2026-08-08T10:10:48.563861Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

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