Paper Citation Record · LEDGER

Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions

As of 17 August 2026, this Paper Citation Record lists 39 of 39 outbound references and 0 inbound Pith citation observations for arXiv:2505.18309.

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pith.paper-citation-record.v1
2505.18309 v1

Coverage vector

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External citation measurements

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Outbound references

Observation 4fefb948-84ac-43da-ae65-70115e4b68b5 · outbound

This paper cites an unresolved cited work.

Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

Reference 1

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

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This paper cites Progress of Theoretical Physics 71(2), 320–326 (1984) https://doi.org/10.

Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Progress of Theoretical Physics 71(2), 320–326 (1984) https://doi.org/10

Reference 3

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This paper cites Progress of Theoretical Physics 72(2), 373–375 (1984) https://doi.org/10.1143/PTP.72.373.

Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Progress of Theoretical Physics 72(2), 373–375 (1984) https://doi.org/10.1143/PTP.72.373

Reference 4

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This paper cites Annual Review of Nuclear and Particle Science 45(45), 429–484 (1995) https://doi.org/10.1146/annurev.ns.45.120195.002241.

Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Annual Review of Nuclear and Particle Science 45(45), 429–484 (1995) https://doi.org/10.1146/annurev.ns.45.120195.002241

Reference 5

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This paper cites Particles 5(3), 225–234 (2022) https://doi.org/10.3390/ particles5030020.

Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Particles 5(3), 225–234 (2022) https://doi.org/10.3390/ particles5030020

Reference 6

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

Reference 7

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This paper cites Physics Letters B 128(3), 137–140 (1983) https://doi.org/10.1016/0370-2693(83)90376-3.

Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Physics Letters B 128(3), 137–140 (1983) https://doi.org/10.1016/0370-2693(83)90376-3

Reference 8

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

Reference 9

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Observation 732942fe-5a7c-4865-b4b8-0d9af9f0dca7 · outbound

This paper cites Compressible 14 Liquid Drop Approaches.

Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Compressible 14 Liquid Drop Approaches

Reference 10

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This paper cites European Physical Journal A 57(10), 296 (2021) https://doi.org/10.1140/epja/s10050-021-00605-6.

Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions European Physical Journal A 57(10), 296 (2021) https://doi.org/10.1140/epja/s10050-021-00605-6

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This paper cites The Astrophysical Journal Supplement Series 204(1), 9 (2012) https://doi.org/ 10.1088/0067-0049/204/1/9.

Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions The Astrophysical Journal Supplement Series 204(1), 9 (2012) https://doi.org/ 10.1088/0067-0049/204/1/9

Reference 12

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

Reference 13

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This paper cites Physics Letters B 485(1-3), 107–114 (2000) https: //doi.org/10.1016/S0370-2693(00)00672-9.

Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Physics Letters B 485(1-3), 107–114 (2000) https: //doi.org/10.1016/S0370-2693(00)00672-9

Reference 14

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Nuclei far from stabilities

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Role of symmetry energy

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This paper cites EPL (Europhysics Letters) 91(3), 32001 (2010) https://doi.org/10.1209/0295-5075/91/32001.

Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions EPL (Europhysics Letters) 91(3), 32001 (2010) https://doi.org/10.1209/0295-5075/91/32001

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions In: Journal of Physics Conference Series

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

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This paper cites arXiv e-prints, 2502–19762 (2025) arXiv:2502.19762.

Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions arXiv e-prints, 2502–19762 (2025) arXiv:2502.19762

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

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This paper cites PhD thesis, University of Illinois, Urbana-Champaign (February 1991).

Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions PhD thesis, University of Illinois, Urbana-Champaign (February 1991)

Reference 37

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Theses, Normandie Universit´ e (September 2023)

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Filling fractions for the formation of nuclear pasta in neutron stars: semiclassical vs liquid-drop predictions Unresolved cited work

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