The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy | Paper Citation Record

Observation 78c824f7-7a32-4b57-a0aa-52c31de2da5f · outbound

This paper cites P., et al.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy P., et al

Reference 1

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:13.209941Z

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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 45e09ed2-a62b-4d04-ac18-434d2e328e22 · outbound

This paper cites P., et al.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy P., et al

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:13.188207Z

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Observation 188163ee-7aec-47c0-b743-c97859efc48d · outbound

This paper cites 2018, PhRvL, 120, 172703.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy 2018, PhRvL, 120, 172703

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:13.169213Z

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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 40f89b80-3c2e-4a4b-a484-faff9bf721d1 · outbound

This paper cites 2013, Sci, 340, 448.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy 2013, Sci, 340, 448

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:13.151846Z

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Observation 09d34e57-86b1-428c-a196-fda684155f54 · outbound

This paper cites 2018, ApJS, 235, 37.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy 2018, ApJS, 235, 37

Reference 5

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:13.131789Z

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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation d42d3372-9661-4fc8-a9e3-10d275561158 · outbound

This paper cites 2017, Ap JL, 850, L34.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy 2017, Ap JL, 850, L34

Reference 6

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:13.111807Z

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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 42a02216-e086-4381-9753-d386cef2d9fb · outbound

This paper cites J., & Sutherland, P.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy J., & Sutherland, P

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:13.090572Z

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Observation bac1b42b-f9d6-4980-a848-26d997596398 · outbound

This paper cites New Neutron Star Equation of State with Quark-Hadron Crossover.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy New Neutron Star Equation of State with Quark-Hadron Crossover

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-14T05:01:10.861650Z

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Observation 03d0e643-1933-4462-965d-b1014170d66b · outbound

This paper cites O., ¨Ozel, F., & G¨ uver, T.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy O., ¨Ozel, F., & G¨ uver, T

Reference 9

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:13.067962Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 7ee58996-95ab-4260-b09f-a6fc11b9169e · outbound

This paper cites 1991, PhRvC, 44, 1892.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy 1991, PhRvC, 44, 1892

Reference 10

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:13.044993Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation cd10c5cd-9564-4601-b53a-eb136e8cd618 · outbound

This paper cites A., & Schwenk, A.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy A., & Schwenk, A

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:13.022716Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation e2efeb9a-c0a6-4109-829f-8748a9e09fd9 · outbound

This paper cites 2004, Nucl.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy 2004, Nucl

Reference 12

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.999637Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 8ca272df-7435-4fa8-bd10-2bb062f16f42 · outbound

This paper cites Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-14T05:01:10.896101Z

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Unavailable: canonical work link unavailable.

Observation df5886b2-9ac2-455c-a584-2eda5f7c663f · outbound

This paper cites an unresolved cited work.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy Unresolved cited work

Reference 14

Resolution: unresolved; raw_fallback, observed 2026-08-14T05:01:12.977296Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 5574d478-730c-4291-92a0-d07cad0480d6 · outbound

This paper cites B., Pennucci, T., Ransom, S.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy B., Pennucci, T., Ransom, S

Reference 15

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.945167Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 0d6f76e7-40a0-455a-bead-bc828f7c5439 · outbound

This paper cites J., Carvajal, J., Newton, W.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy J., Carvajal, J., Newton, W

Reference 16

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.913305Z

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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 8ab81db6-05ec-4dfe-9c6d-4a326e50814d · outbound

This paper cites J., Newton, W.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy J., Newton, W

Reference 17

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.872495Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 966d3107-d4fd-474d-9ca6-6769779daf8a · outbound

This paper cites J., Piekarewicz, J., & Horowitz, C.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy J., Piekarewicz, J., & Horowitz, C

Reference 18

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.837233Z

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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 2f37e773-4075-4a7d-a8e5-ba387766869f · outbound

This paper cites The impact of the crust equation of state on the analysis of GW170817.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy The impact of the crust equation of state on the analysis of GW170817

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-14T05:01:10.949840Z

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Unavailable: canonical work link unavailable.

Observation 03747d82-a30c-4801-98fa-171b9cd5476e · outbound

This paper cites & Rutledge, R.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy & Rutledge, R

Reference 20

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.814365Z

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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 55fc427c-0085-4bc3-9ba1-99bfa8338661 · outbound

This paper cites 2008, ApJ, 677, 1216.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy 2008, ApJ, 677, 1216

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-14T05:01:10.975100Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5d13be7a-cb9c-4f31-97f4-333619f7a50d · outbound

This paper cites D., Lang, R.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy D., Lang, R

Reference 22

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.776621Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 4d68749f-dd91-422f-9960-fec50e42ee76 · outbound

This paper cites M., Lim, Y., Kwak, K., Hyun, C.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy M., Lim, Y., Kwak, K., Hyun, C

Reference 23

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.744735Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 5cda1b1c-3deb-44ff-9e52-8d94605d0a1a · outbound

This paper cites 2004, PhRvC, 70, 065804.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy 2004, PhRvC, 70, 065804

Reference 24

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.715652Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 051dfc82-c200-4361-ae36-c16516431d65 · outbound

This paper cites 2007, PhRvC, 76, 025801.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy 2007, PhRvC, 76, 025801

Reference 25

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.688381Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 5588b333-561d-400d-b04e-04aa7d1c7bc8 · outbound

This paper cites M., & Prakash, M.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy M., & Prakash, M

Reference 26

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.663914Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 8c4403c0-7919-40d9-8e69-1e098c298e20 · outbound

This paper cites M., & Prakash, M.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy M., & Prakash, M

Reference 27

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.636433Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 9e38ce26-496e-4cbe-a576-3ed72ba2d83e · outbound

This paper cites M., & Prakash, M.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy M., & Prakash, M

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-14T05:01:11.023746Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4bcf2e3a-27da-45bc-870a-08b89e579218 · outbound

This paper cites M., & Steiner, A.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy M., & Steiner, A

Reference 29

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.594687Z

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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 0de90b8f-6fa1-4766-a185-b0390e7ccc65 · outbound

This paper cites A., & Steiner, A.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy A., & Steiner, A

Reference 30

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.561682Z

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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation f638b424-2acb-4c41-a590-f95795a23543 · outbound

This paper cites A., & Han, X.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy A., & Han, X

Reference 31

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.524883Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 8550e3fe-4382-4fd4-a49d-e7ec92477125 · outbound

This paper cites an unresolved cited work.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy Unresolved cited work

Reference 32

Resolution: unresolved; raw_fallback, observed 2026-08-14T05:01:12.492149Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 44925cbf-c7ba-4152-a4d6-2cc9fe1443ea · outbound

This paper cites A., Krastev, P.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy A., Krastev, P

Reference 33

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.467274Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 06d709c3-1e9d-45a0-9ac8-1ca0c849416a · outbound

This paper cites Consistent Skyrme parametrizations constrained by GW170817.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy Consistent Skyrme parametrizations constrained by GW170817

Reference 34

Resolution: verified exact; local_arxiv, observed 2026-08-14T05:01:11.537712Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation b018a17b-92bd-47a4-8b2e-8350f489865b · outbound

This paper cites K., Kumar, B., & Patra, S.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy K., Kumar, B., & Patra, S

Reference 35

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.440270Z

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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 7748e8fa-21a6-4c07-8f0e-8fdb6865f3fe · outbound

This paper cites an unresolved cited work.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy Unresolved cited work

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-14T05:01:11.097620Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 55a6d218-3fff-4af2-a468-34094a6eba2e · outbound

This paper cites 2011, Astrophys.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy 2011, Astrophys

Reference 37

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.399121Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 5537b4f2-9144-4966-b98c-c8db4fc7ef27 · outbound

This paper cites C., & Lamb, F.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy C., & Lamb, F

Reference 38

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.368231Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 4921e81b-7ae4-465d-8483-dd93472c559b · outbound

This paper cites R., W eih, L.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy R., W eih, L

Reference 39

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.347645Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation ec18ba2e-0ca5-4f62-9452-9cf77689cafd · outbound

This paper cites 2019, PhRvC, 99, 052802 N¨ attil¨ a, J., Miller, M.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy 2019, PhRvC, 99, 052802 N¨ attil¨ a, J., Miller, M

Reference 40

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.325550Z

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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation d08cf8eb-8a9d-4a59-a5be-611510eed63f · outbound

This paper cites F., & Poutanen, J.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy F., & Poutanen, J

Reference 41

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.301672Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 53fc53e6-1446-4ed1-b70d-031a8a9fcd7d · outbound

This paper cites W., & Vautherin, D.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy W., & Vautherin, D

Reference 42

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.272751Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation f281373c-064c-4f7e-91c0-b1bec4712ca7 · outbound

This paper cites 2017, Rev.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy 2017, Rev

Reference 43

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.248510Z

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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 8685ede2-97fc-45fe-919f-85aa7847b48e · outbound

This paper cites 1939, Phys.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy 1939, Phys

Reference 44

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.220514Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 0aa4bbea-1b4c-450e-a574-dba561de7601 · outbound

This paper cites an unresolved cited work.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy Unresolved cited work

Reference 45

Resolution: unresolved; raw_fallback, observed 2026-08-14T05:01:12.192479Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 867ee3e3-3c85-4014-9c46-43c7264347f8 · outbound

This paper cites Nuclear Astrophysics in the New Era of Multimessenger Astronomy.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy Nuclear Astrophysics in the New Era of Multimessenger Astronomy

Reference 46

Resolution: metadata mismatch; local_arxiv, observed 2026-08-14T05:01:11.489509Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 8ed42dde-ef11-4bae-9619-1eaa080173a5 · outbound

This paper cites an unresolved cited work.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy Unresolved cited work

Reference 47

Resolution: unresolved; raw_fallback, observed 2026-08-14T05:01:12.162509Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation f25eb370-e49e-488c-8a16-4dafd44c9c46 · outbound

This paper cites 2019, Eur.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy 2019, Eur

Reference 48

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.139349Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 12cf5d3e-9096-4e88-a110-59c542d7cec5 · outbound

This paper cites A., ¨Ozel, F., & Psaltis, D.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy A., ¨Ozel, F., & Psaltis, D

Reference 49

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.115653Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 4a7f61f3-84e4-4045-94f7-30550b4e4f82 · outbound

This paper cites an unresolved cited work.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy Unresolved cited work

Reference 50

Resolution: unresolved; raw_fallback, observed 2026-08-14T05:01:12.097109Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 42d9d783-61d0-4b50-8df5-db050d381b4b · outbound

This paper cites R., & W eih, L.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy R., & W eih, L

Reference 51

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.064113Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation b2edd44f-2371-4e35-add4-bd7e32640ce8 · outbound

This paper cites L., & Tsokaros, A.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy L., & Tsokaros, A

Reference 52

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.040704Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 9a80de6e-16e0-4427-bc62-984de59d8610 · outbound

This paper cites W., et al.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy W., et al

Reference 53

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:12.012039Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 80007c3a-3083-48e9-8165-c95ee2f1d32a · outbound

This paper cites 2017, PhRvD, 96, 123012.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy 2017, PhRvD, 96, 123012

Reference 54

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:11.990575Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation b7f9dd60-932a-4956-a572-4443868bf1b1 · outbound

This paper cites 2019, PhRvD, 100, 023015.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy 2019, PhRvD, 100, 023015

Reference 55

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:11.965006Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 87077700-e897-4713-844f-b3cc5116be66 · outbound

This paper cites M., & Col` o G.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy M., & Col` o G

Reference 56

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:11.944823Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 23e6319f-8d11-4878-9183-9cb6ad7458f1 · outbound

This paper cites W., Lattimer, J.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy W., Lattimer, J

Reference 57

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:11.920671Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 7d6d2e73-9f64-4879-bda0-07b42a708603 · outbound

This paper cites F.,Poutanen, J., Klochkov, D., & W erner, K.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy F.,Poutanen, J., Klochkov, D., & W erner, K

Reference 58

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:11.902095Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 8adbbafb-3e88-4840-8bd2-fca73eb422da · outbound

This paper cites M., Ohnishi, A., & Kolomeitsev, E.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy M., Ohnishi, A., & Kolomeitsev, E

Reference 59

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:11.869853Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 042519b4-7a77-4690-a855-15a0865d56f6 · outbound

This paper cites 2018, PhRvC, 98, 045804.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy 2018, PhRvC, 98, 045804

Reference 60

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:11.850161Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 3abd8997-35d2-45ac-8c9b-ba9d24fde2c0 · outbound

This paper cites an unresolved cited work.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy Unresolved cited work

Reference 61

Resolution: unresolved; raw_fallback, observed 2026-08-14T05:01:11.828154Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation e9aa435f-1f22-49c9-ada3-a67e865d1dd6 · outbound

This paper cites Symmetry energy at supra-saturation densities via the Gravitational Waves from GW170817.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy Symmetry energy at supra-saturation densities via the Gravitational Waves from GW170817

Reference 62

Resolution: verified exact; local_arxiv, observed 2026-08-14T05:01:11.460557Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 67db6591-56a7-4dc8-bf96-27d704a2ca58 · outbound

This paper cites Insights on Skyrme parameters from GW170817.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy Insights on Skyrme parameters from GW170817

Reference 63

Resolution: verified exact; local_arxiv, observed 2026-08-14T05:01:11.429825Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation d6aa6c13-ab1d-411d-8d90-300b9edb379c · outbound

This paper cites W., Li, B.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy W., Li, B

Reference 64

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:11.807881Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 3267fb2f-f100-42d5-93a9-6a317ebeabf0 · outbound

This paper cites B., Cai, B.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy B., Cai, B

Reference 65

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:11.789225Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 0bb5e5b8-da89-49d3-9558-510abbe6285d · outbound

This paper cites B., Li, B.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy B., Li, B

Reference 66

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:11.750671Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 331d5d88-55d9-4a70-9e96-b3f58c2aa200 · outbound

This paper cites B., & Li, B.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy B., & Li, B

Reference 67

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:11.715207Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation ee40ac0d-b5ce-4230-9097-8d24dd5ddb75 · outbound

This paper cites Q., & Lattimer, J.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy Q., & Lattimer, J

Reference 68

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:11.680628Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 7b635fe7-5b66-4cae-bb8c-07dd737ea39c · outbound

This paper cites P., Zhou, X., & Li, A.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy P., Zhou, X., & Li, A

Reference 69

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:11.657394Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 23614b5d-1c66-49f5-abea-4a2b068c2ae3 · outbound

This paper cites W., & Zhang, Z.

The key factor to determine the relation between radius and tidal deformability of neutron stars: slope of symmetry energy W., & Zhang, Z

Reference 70

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T05:01:11.630986Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

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Reference resolution

Outbound references

Pith citing papers