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Neutron stars in $f(Q) = Q +\xi Q^2$ gravity

As of 18 August 2026, this Paper Citation Record lists 61 of 61 outbound references and 0 inbound Pith citation observations for arXiv:2607.04596.

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pith.paper-citation-record.v1
2607.04596 v1

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measured 61 of 61 reference resolution

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61 of 61 outbound references displayed

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Outbound references

Observation 48722d5a-b084-481a-b2bb-9c0eef238664 · outbound

This paper cites Will, The Confrontation between General Relativity and Experiment, Living Rev.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Will, The Confrontation between General Relativity and Experiment, Living Rev

Reference 1

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Observation 14d96086-cbda-4677-b5c4-bf375c4c750e · outbound

This paper cites Comparing Equivalent Gravities: common features and differences.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Comparing Equivalent Gravities: common features and differences

Reference 2

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Observation 65bcbe8b-dea5-4b82-ac65-be3b5b062ff7 · outbound

This paper cites Riess et al., Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant, Astron.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Riess et al., Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant, Astron

Reference 3

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Observation df7be77a-5e56-416e-b50a-72d759fd8515 · outbound

This paper cites Peebles and B.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Peebles and B

Reference 4

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:1e416efc50c501b3117cd715f6f1ff3fafdd2c8c3710cffb0a82e7fb17cedb6b

Observation a2b48f01-bd40-43dd-a128-8733cc15e4c9 · outbound

This paper cites Sotiriou and V.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Sotiriou and V

Reference 5

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Observation d177fe2e-c3a3-481a-8ea0-d8e59f173b18 · outbound

This paper cites Jim´ enez et al., The Geometrical Trinity of Gravity, Universe 5, 173 (2019).

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Jim´ enez et al., The Geometrical Trinity of Gravity, Universe 5, 173 (2019)

Reference 6

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:08ebbca34b9bfd306669b3b33438400c3cfb5ba513b22dd46147a695c9e200b5

Observation 8dc188c8-ab8a-49ca-b69e-a03fd176ee88 · outbound

This paper cites Aldrovandi and J.G.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Aldrovandi and J.G

Reference 7

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:78a184749b4c3b0a31be2e002db170df4096e70ba4cc13e84bd0a8bd183378ef

Observation 6e123b03-1c5d-4659-a574-f4b695d6261f · outbound

This paper cites Teleparallel Gravity: From Theory to Cosmology.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Teleparallel Gravity: From Theory to Cosmology

Reference 8

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:1a9181c978f536cd91f9758cebaa22bef806efc8993da4c330df1685bdee7f38

Observation b48b2b9f-9bcb-4c5c-879f-81412a57b608 · outbound

This paper cites Cai et al., f(T) teleparallel gravity and cosmology, Rept.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Cai et al., f(T) teleparallel gravity and cosmology, Rept

Reference 9

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:abdb23d70e8351fa9b20174c1eee311bc66d10956fdc07f5f3b0e066c45af190

Observation 98bd9032-4b97-4363-a9e3-e406dee8a22b · outbound

This paper cites Modified teleparallel gravity: inflation without inflaton.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Modified teleparallel gravity: inflation without inflaton

Reference 10

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:5d29aee8f51902d0c9e18e64e791a944551a86a9a911e2bfdef828f9d82567e8

Observation f5be3535-020a-4af1-a88f-50eba88e706c · outbound

This paper cites Einstein's Other Gravity and the Acceleration of the Universe.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Einstein's Other Gravity and the Acceleration of the Universe

Reference 11

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:720e024e3e849846f23dfc4ff8155220441de8befef42a8bdac9e7b716b91a96

Observation 29d44d84-b3ec-4b05-aae8-6ebb4d2cf7d0 · outbound

This paper cites Accelerating universe from F(T) gravity.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Accelerating universe from F(T) gravity

Reference 12

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:ee152d42755d0e74c1a231b9daf8844bf30e7106359a4f59f5cab1bdb729a7f0

Observation 3fe12d2b-45d5-4db8-a991-0af93c9514ca · outbound

This paper cites Karami and A.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Karami and A

Reference 13

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:8a6e62e517c0abbb5bc9b5deb4d3b9e0f175280810d142755132c6b7fe02859c

Observation 4d183fc4-6a5d-4079-a7e0-eebac7a97d90 · outbound

This paper cites Ganiou et al., Strong magnetic field effects on neutron stars within f(T) theory of gravity, Eur.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Ganiou et al., Strong magnetic field effects on neutron stars within f(T) theory of gravity, Eur

Reference 14

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Observation 7df54e6d-ed5f-41ab-adf3-07dae2a4b6bd · outbound

This paper cites Kpadonou, M.J.S.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Kpadonou, M.J.S

Reference 15

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:3e697ca37cf3f734e52aff721ea9c7a42c1a85fc446c902812ef491bf4ba3b35

Observation 4e8deda9-1e21-41aa-a8c0-4277420be2f2 · outbound

This paper cites Pace and J.L.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Pace and J.L

Reference 16

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Observation be97b22a-3a5d-4d6c-a484-fa86cc890931 · outbound

This paper cites Iliji´ c and M.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Iliji´ c and M

Reference 17

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Observation 85a7bb1b-611b-4b1d-902d-19a64aa7a304 · outbound

This paper cites B¨ ohmer, A.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity B¨ ohmer, A

Reference 18

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Observation b86e22ee-591e-47ab-8d74-291c91841284 · outbound

This paper cites Pace, J.L.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Pace, J.L

Reference 19

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:b023b3b370c38a12a8727b48b29f81cdeb0b0580afd6a44f280d5113f0bb6027

Observation 8b833d0f-c19c-4d35-8178-88b21b9625a2 · outbound

This paper cites Solving Tolman-Oppenheimer-Volkoff equations in $f(T)$ gravity: a novel approach.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Solving Tolman-Oppenheimer-Volkoff equations in $f(T)$ gravity: a novel approach

Reference 20

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:cf44c1f94f363cc3eeda5410b385922a8bfc1e0978245ce3d8cf9f1b9e48d6c8

Observation b3bf096a-5109-43cc-a4ff-3e5c4ae8fbe4 · outbound

This paper cites Solving Tolman-Oppenheimer-Volkoff equations in $f(T)$ gravity: a novel approach applied to polytropic equations of state.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Solving Tolman-Oppenheimer-Volkoff equations in $f(T)$ gravity: a novel approach applied to polytropic equations of state

Reference 21

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:15af68b37a9b595ccfd9312ec901b32e9d7897415046966053ec1187817e2761

Observation a344cedd-27f2-47ed-86bb-64dece2837f1 · outbound

This paper cites Solving Tolman-Oppenheimer-Volkoff equations in f(T) gravity: a novel approach applied to some realistic equations of state.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Solving Tolman-Oppenheimer-Volkoff equations in f(T) gravity: a novel approach applied to some realistic equations of state

Reference 22

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:4d23989a2ca42725e82bcf98032966f69d2c09bf5dff26866036cfb64984458e

Observation 7c29fac2-54bd-4ab7-980a-323bf50b0cb4 · outbound

This paper cites Mass of compact stars in f(T) gravity.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Mass of compact stars in f(T) gravity

Reference 23

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:66c45977a50d9b24b54fb496e5c857f042e42db4a7ec84fd7a0658ef12d697c8

Observation 9646e33e-1165-479b-bf30-bee347f8be48 · outbound

This paper cites de Araujo and H.G.M.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity de Araujo and H.G.M

Reference 24

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:9c6549ee51be4b196ac2c53a3eb1e329b959e291cce62917ae6264bb469d9f6c

Observation 5ce6a72d-32ea-44dc-be58-2d4d74068dea · outbound

This paper cites A flat FLRW dark energy model in f(Q,C)-gravity theory with observational constraints.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity A flat FLRW dark energy model in f(Q,C)-gravity theory with observational constraints

Reference 25

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:28f670e7945a1593167b3e83c60ed431d23f82fda1091ac529e08b6d6662aef6

Observation b165941a-a300-4b7a-88fb-b02ffead1b67 · outbound

This paper cites Cosmological observational constraints on the power law $f(Q)$ type modified gravity theory.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Cosmological observational constraints on the power law $f(Q)$ type modified gravity theory

Reference 26

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:359a692ac72d87c65e41354cef2c2a8075b37d512bbcf7c8e1d290f2bdb00fab

Observation b89eb54f-603e-4b14-b154-056e759aad90 · outbound

This paper cites Quintessence scalar field model in Weyl-type $f(Q,T)$ Gravity with $w_D-w'_D$ analysis.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Quintessence scalar field model in Weyl-type $f(Q,T)$ Gravity with $w_D-w'_D$ analysis

Reference 27

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Observation 64408258-635e-469b-9ce7-1863e0476fce · outbound

This paper cites Cosmological implications of the constant jerk parameter in $f(Q,T)$ gravity theory.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Cosmological implications of the constant jerk parameter in $f(Q,T)$ gravity theory

Reference 28

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:ba01daf91f005833baed8aafdb4f8a524441bd9a90a35fb1708cacf9882e56d2

Observation 90cc2861-b5d6-4581-9269-949109d61541 · outbound

This paper cites Adak et al., Symmetric Teleparallel Gravity: Some Exact Solutions And Spinor Couplings, IJMP A, 28, 1350167 (2013).

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Adak et al., Symmetric Teleparallel Gravity: Some Exact Solutions And Spinor Couplings, IJMP A, 28, 1350167 (2013)

Reference 29

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Observation 95ae6542-32e3-4880-9fcf-8783edf09de6 · outbound

This paper cites Scalar induced gravitational waves in symmetric teleparallel gravity with a parity-violating term.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Scalar induced gravitational waves in symmetric teleparallel gravity with a parity-violating term

Reference 30

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:23b59e9cfdca986a444caa868d36a42bd306d70555d479d6110dc7f1faf7fea0

Observation cbdb7d8a-f91b-48f8-8c55-5019f30e4ca0 · outbound

This paper cites Hamiltonian Analysis of $f(Q)$ Gravity and the Failure of the Dirac-Bergmann Algorithm for Teleparallel Theories of Gravity.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Hamiltonian Analysis of $f(Q)$ Gravity and the Failure of the Dirac-Bergmann Algorithm for Teleparallel Theories of Gravity

Reference 31

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:68c8e88dbc0b23d6527e058e882e66c73d23ed4436a9f133b8e9d59d8527358f

Observation 4006ceab-2902-4feb-a4cb-81a045fd232e · outbound

This paper cites Geometry and covariance of symmetric teleparallel theories of gravity.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Geometry and covariance of symmetric teleparallel theories of gravity

Reference 32

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Observation 0c72e179-b983-42eb-ae98-49cabf00b3c5 · outbound

This paper cites Constraining f(Q) Cosmology with Standard Sirens.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Constraining f(Q) Cosmology with Standard Sirens

Reference 33

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:64c7d3aa782f3b13014b783117e655a43f3f3a14e8f5bb44290972d77d2d2068

Observation baf039d6-bbf4-444e-a8fa-f8f80d11da4d · outbound

This paper cites A class of static spherically symmetric solutions in $f(Q)$-gravity.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity A class of static spherically symmetric solutions in $f(Q)$-gravity

Reference 34

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:a40dbb8cb7306222f20c91796764776b7c6a63bb2e0556fbeac67350a4c3f522

Observation 2789dce7-b5ce-4ccc-8bc4-45676469270b · outbound

This paper cites Anisotropic Strange Star Model Beyond Standard Maximum Mass Limit by Gravitational Decoupling in $f(Q)$ Gravity.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Anisotropic Strange Star Model Beyond Standard Maximum Mass Limit by Gravitational Decoupling in $f(Q)$ Gravity

Reference 35

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:5028d9b269b0da666eb131e3ad12c93d9bc11c1e0548f9491563d58ad59330e7

Observation 37ba75d1-0b0a-42a4-9da8-f388861ae4c9 · outbound

This paper cites Influence of three parameters on maximum mass and stability of strange star under linear $f(Q)-$action.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Influence of three parameters on maximum mass and stability of strange star under linear $f(Q)-$action

Reference 36

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:b06fc0c5937ec7ea53627adee7c2fae0b39b7e6c02717bc2742a308578c8072a

Observation ab4c8e76-0fed-4758-89f7-106d9fd491cc · outbound

This paper cites Shekh et al., Models of f(Q) gravity with electromagnetic field, arXiv:2309.15853 [gr-qc] (2023).

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Shekh et al., Models of f(Q) gravity with electromagnetic field, arXiv:2309.15853 [gr-qc] (2023)

Reference 37

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:6813dd8e19a47206ad04daecf964e748aa7a5db24869a09101ca5d62cd308781

Observation 6ac76f3d-cc44-42c3-a733-6646c55f9aa9 · outbound

This paper cites The role of the boundary term in $f(Q,B)$ symmetric teleparallel gravity.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity The role of the boundary term in $f(Q,B)$ symmetric teleparallel gravity

Reference 38

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:de8a480f0d43b923c5adf083ba3235e89ba65e330a290b93af7d46b07e32ec46

Observation 9ddd9028-6192-4808-903d-95b08e6c9761 · outbound

This paper cites Review on $f(Q)$ Gravity.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Review on $f(Q)$ Gravity

Reference 39

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:b50895b09014c023634f3171fbb206aa286dc6b9d916acee4fa41fac2f006ad3

Observation 7ffff59a-e6af-4267-906c-ea204146d93b · outbound

This paper cites Errehymy et al., Anisotropic electrically charged stars in f(Q) symmetric teleparallel gravity, Eur.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Errehymy et al., Anisotropic electrically charged stars in f(Q) symmetric teleparallel gravity, Eur

Reference 40

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:5c425ff74e67d37b83c2d42c1a24ec7974dff51656b3bc67683595e30e5a134f

Observation 3dcdde10-1a1e-4500-af7d-1cd72762f0be · outbound

This paper cites Lin and X.H.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Lin and X.H

Reference 41

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:d64ef077fdd6209ff637f4bafb6bd2f7b8772f1177ea1e385220d3091af38cb6

Observation 4129c091-9d7c-4f93-8fae-7bf3da4a55e7 · outbound

This paper cites Gakis et al., Conformal gravity and transformations in the symmetric teleparallel framework, Phys.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Gakis et al., Conformal gravity and transformations in the symmetric teleparallel framework, Phys

Reference 42

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:9fc7320f0fcccbff6bc22adca056c6657e174d827ca7ec22387652ac40990ade

Observation 54518a7a-847a-4a42-af1e-43f75f4ca121 · outbound

This paper cites Covariant formulation of f(Q) theory.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Covariant formulation of f(Q) theory

Reference 43

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:90e780be335669ac339318a3f76f9677f7189966fe522358deee762aaaa120fd

Observation fc8cbbef-6451-43d2-bde7-483324d6350b · outbound

This paper cites Buchdahl quark stars within $f(Q)$ theory.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Buchdahl quark stars within $f(Q)$ theory

Reference 44

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:bf824a43eb7112aacfcb3fbc7a151d6b9b89ac8254efa8566dcce89014d86874

Observation 7084c11b-4d58-4761-b226-0490a207376f · outbound

This paper cites Static and spherically symmetric solutions in f(Q) gravity.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Static and spherically symmetric solutions in f(Q) gravity

Reference 45

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:139ba365b5675977473c50a08920d1f7406700cc9b9c2b805ee17b92f0194c17

Observation cffafec0-6246-42d9-b1de-97aee820813d · outbound

This paper cites Jim´ enez et al.,Cosmology in f(Q) geometry, Phys.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Jim´ enez et al.,Cosmology in f(Q) geometry, Phys

Reference 46

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:3c1acdc5ce90d9a0abe6c7f3c15115396650c1de6416ee9ed1886a7d78d3f681

Observation f3509890-6861-4090-b3fd-197e897fc5ce · outbound

This paper cites Physical Characteristics and Maximum Allowable Mass of Hybrid Star in the Context of $f(Q)$ Gravity.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Physical Characteristics and Maximum Allowable Mass of Hybrid Star in the Context of $f(Q)$ Gravity

Reference 47

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:eb236de42d84970bf8e6d006ec8910bd388a7c83f44f4a54312e9c3e528a5998

Observation 66783600-8538-4c56-b171-2c187d273d32 · outbound

This paper cites On the viability of $f(Q)$ gravity models.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity On the viability of $f(Q)$ gravity models

Reference 48

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:7dc7147843237adde540058d5f8f48c0c04f5bc89bd0282d6c68217aafb53990

Observation b9b0eb70-7e23-424f-8088-1fc74be1be1f · outbound

This paper cites Gravastar in the Framework of Symmetric Teleparallel Gravity.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Gravastar in the Framework of Symmetric Teleparallel Gravity

Reference 49

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:cffe01d55ed137daba4ca6ebcaec049cb34fe1a23f86dc73af075d1747fa715e

Observation 606e71a2-2f47-4542-b4c0-83332a9f906e · outbound

This paper cites Statistical and Observation Comparison of Weyl-Type $f(Q,T)$ Models with the $\Lambda$CDM Paradigm.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Statistical and Observation Comparison of Weyl-Type $f(Q,T)$ Models with the $\Lambda$CDM Paradigm

Reference 50

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:5b0aa751f8d2546d895c7afd815146752129d9a68dceb8a2d2687ec553773bd1

Observation 94c5d46e-6a20-4896-b914-e34ddcc92f93 · outbound

This paper cites de Araujo and H.G.M.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity de Araujo and H.G.M

Reference 51

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:1ca96f087643bbb33064a21578fb70210aa4603b66fac70e3c1dbbb9ee924257

Observation e137d69e-7a5c-4118-a194-3b37c12637fd · outbound

This paper cites Buchdahl compactness limit and gravitational field energy.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Buchdahl compactness limit and gravitational field energy

Reference 52

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:d234f9fbd909731c77f5e4f17af69a3a2579f49d74b103ab17c59b438c84cc74

Observation 99ea5c56-cf29-4022-afca-cae854342f39 · outbound

This paper cites an unresolved cited work.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Unresolved cited work

Reference 53

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:0ba85fad4e207584e95e14aaa52f8b13aa5d745ddc0f48b94ebc16495ca039a5

Observation b2da20d3-0928-4c9a-a8cc-cf83dff26835 · outbound

This paper cites Weighing massive neutron star with screening gravity: A look on PSR J0740+6620 and GW190814 secondary component.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Weighing massive neutron star with screening gravity: A look on PSR J0740+6620 and GW190814 secondary component

Reference 54

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:e4fb7cafa88ff9b6ccf275cfbe5f5e05ee104ea701cd538c7ca602c5f0aee203

Observation e6c19435-46a4-42eb-b0e4-ed66ee4076b6 · outbound

This paper cites GW190814: Gravitational Waves from the Coalescence of a 23 M$_\odot$ Black Hole with a 2.6 M$_\odot$ Compact Object.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity GW190814: Gravitational Waves from the Coalescence of a 23 M$_\odot$ Black Hole with a 2.6 M$_\odot$ Compact Object

Reference 55

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:42fb7941a00a66f54913609217d0f855d0a150e06c602132c13c2f507b2b016b

Observation 4007db91-9f57-4c2e-b3cd-61b7e43119bb · outbound

This paper cites an unresolved cited work.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Unresolved cited work

Reference 56

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:3dbed740f2706ec7569d6a93e85a9b2c4923211a6877dc84ab8c6c40fca433f3

Observation 2ab08eb8-7019-4d85-adc8-77124bdef79d · outbound

This paper cites Cromartie et al., Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar, Nat Astron 4, 72 (2020).

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Cromartie et al., Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar, Nat Astron 4, 72 (2020)

Reference 57

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:cda8c6f05d0f3e6c682fa1057fd73550951dc4aeee3ac858996b5e1ff85c21c7

Observation 5ce3b4cd-6d81-4989-b7a5-92b07a66d9c9 · outbound

This paper cites Antoniadis et al., A massive pulsar in a compact relativistic binary, Science, 340, 1233232 (2013).

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Antoniadis et al., A massive pulsar in a compact relativistic binary, Science, 340, 1233232 (2013)

Reference 58

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:3d81bc08fa2939927daa8c3ba08e5c11bfbc00f6d773cb5658693cf44c9f5842

Observation 8de279ee-5c1b-458d-b8d7-6f0eeb3d62a6 · outbound

This paper cites an unresolved cited work.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Unresolved cited work

Reference 59

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:20dd230275f052605568494d378cbced78088b70a33ac3e935ac25b19349608d

Observation c7247f7e-42cd-4ad5-ae88-b602733de685 · outbound

This paper cites Abbott et al., Properties of the binary neutron star merger GW170817, Physical Review X, 9, 011001 (2019).

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Abbott et al., Properties of the binary neutron star merger GW170817, Physical Review X, 9, 011001 (2019)

Reference 60

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:3f3eec87a5759964ce40f5ba25b0ec940a7212749fff8ff976585d4b98b933b8

Observation 988bc9c7-7025-4395-82fb-73b1f6f4338a · outbound

This paper cites Abbott et al., GW190425: Observation of a Compact Binary Coalescence with Total Mass ∼ 3.4 M⊙, Astrophys.

Neutron stars in $f(Q) = Q +\xi Q^2$ gravity Abbott et al., GW190425: Observation of a Compact Binary Coalescence with Total Mass ∼ 3.4 M⊙, Astrophys

Reference 61

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source=pdf_text observed=2026-07-11T16:40:07.642828Z digest=sha256:448d4683e9087105b5b1ff6c9d68c7d92b11063f38d727de67d25b18b01f73c7

Pith citing papers

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