Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves | Paper Citation Record

Observation 2ac3dfbe-cf00-4602-967a-2fff21afe0cf · outbound

This paper cites Einstein, Die Feldgleichungen der Gravitation , Sitzungsberichte der Königlich Preussischen Akademie der Wissenschaften (1915) 844.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Einstein, Die Feldgleichungen der Gravitation , Sitzungsberichte der Königlich Preussischen Akademie der Wissenschaften (1915) 844

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Observation 996fc976-9d20-4e65-82f7-a35837a62686 · outbound

This paper cites Holberg, Sirius B and the Measurement of the Gravitational Redshift , Journal for the History of Astronomy 41 (2010) 41.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Holberg, Sirius B and the Measurement of the Gravitational Redshift , Journal for the History of Astronomy 41 (2010) 41

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Observation 88f4468d-e749-4c5b-8f37-fa9e172c2dd0 · outbound

This paper cites Hulse and J.H.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Hulse and J.H

Reference 3

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Observation 4534fcf1-590f-41ee-b969-f1aa4dd06a3c · outbound

This paper cites Clark and D.M.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Clark and D.M

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Observation d593c43b-8f4f-4364-a394-959e2cfd680b · outbound

This paper cites Damour and N.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Damour and N

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Observation c1ea4b44-81d7-4467-ac90-1d4d1e6e38de · outbound

This paper cites Damour and N.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Damour and N

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Observation 74e7e254-d2df-4f6f-bb82-7b3fd9f5b6f9 · outbound

This paper cites The International Pulsar Timing Array: Second data release.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves The International Pulsar Timing Array: Second data release

Reference 7

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Observation af5ee59c-6128-4d8c-9815-1cf76bac7a37 · outbound

This paper cites Estimating the sensitivity of pulsar timing arrays.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Estimating the sensitivity of pulsar timing arrays

Reference 8

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Observation 87729f96-e191-4c99-a1f2-67a9b755cc1b · outbound

This paper cites Observation of Gravitational Waves from a Binary Black Hole Merger.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Observation of Gravitational Waves from a Binary Black Hole Merger

Reference 9

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Observation 3b5f75cc-bf45-4751-8286-f6e6ad1ea0ec · outbound

This paper cites GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence

Reference 10

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Observation 2e7dfac8-abee-4823-8be4-b29fdab4f979 · outbound

This paper cites GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves GW170104: Observation of a 50-Solar-Mass Binary Black Hole Coalescence at Redshift 0.2

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Observation 62c3abcd-eb7f-4d4e-a564-065bf37f2c46 · outbound

This paper cites GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence

Reference 12

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Observation 1ccb6f3d-5bae-44ad-b76e-c32aa61e58bf · outbound

This paper cites GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence

Reference 13

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Observation a2a438e5-4c01-449b-813e-fc98d819b32d · outbound

This paper cites GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

Reference 14

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Observation 981fcab1-7bb3-40da-b184-0eab5856e068 · outbound

This paper cites The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background

Reference 15

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Observation 83ffaec8-9426-4281-9514-6697304302f1 · outbound

This paper cites All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO and Advanced Virgo O3 data.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves All-sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO and Advanced Virgo O3 data

Reference 16

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This paper cites Drop in the hard pulsed fraction and a candidate cyclotron line in IGR J16320-4751 seen by NuSTAR.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Drop in the hard pulsed fraction and a candidate cyclotron line in IGR J16320-4751 seen by NuSTAR

Reference 17

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Observation 51b913bb-99b1-466f-94b3-eafd3ded2878 · outbound

This paper cites Einstein's Discovery of Gravitational Waves 1916-1918.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Einstein's Discovery of Gravitational Waves 1916-1918

Reference 18

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Observation 848fe798-5d03-47cd-8902-f36934a7d54a · outbound

This paper cites Einstein, Die Grundlage der allgemeinen Relativit¨ atstheorie, Annalen der Physik 354 (1916) 769.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Einstein, Die Grundlage der allgemeinen Relativit¨ atstheorie, Annalen der Physik 354 (1916) 769

Reference 19

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Observation a646abda-9d71-4c18-b483-99021fca52fa · outbound

This paper cites Einstein, N¨ aherungsweise Integration der Feldgleichungen der Gravitation, Sitzungsberichte der Königlich Preussischen Akademie der Wissenschaf ten (1916) 688.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Einstein, N¨ aherungsweise Integration der Feldgleichungen der Gravitation, Sitzungsberichte der Königlich Preussischen Akademie der Wissenschaf ten (1916) 688

Reference 20

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Observation a7c75a58-99f5-42fb-9bd6-ad6f59da4492 · outbound

This paper cites Einstein, ¨Uber Gravitationswellen, Sitzungsberichte der Königlich Preussischen Akademie der Wissenschaften (1918) 154.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Einstein, ¨Uber Gravitationswellen, Sitzungsberichte der Königlich Preussischen Akademie der Wissenschaften (1918) 154

Reference 21

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Observation 86442b03-71c2-454e-bbbf-b7e05cc512d7 · outbound

This paper cites Eddington, The Propagation of Gravitational Waves , Proceedings of the Royal Society of London Series A 102 (1922) 268.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Eddington, The Propagation of Gravitational Waves , Proceedings of the Royal Society of London Series A 102 (1922) 268

Reference 22

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Observation 7a9e9d8a-ad8d-484f-a5d0-9cbd68ffa828 · outbound

This paper cites Eddington, The Mathematical Theory of Relativity , Cambridge University Press, Cambridge, England (1923).

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Eddington, The Mathematical Theory of Relativity , Cambridge University Press, Cambridge, England (1923)

Reference 23

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Observation ecdaee86-9005-4fba-8225-9f6961b64182 · outbound

This paper cites Gravitational waves from extreme mass ratio inspirals: Challenges in mapping the spacetime of massive, compact objects.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Gravitational waves from extreme mass ratio inspirals: Challenges in mapping the spacetime of massive, compact objects

Reference 24

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Observation 8effaf5a-dd38-45be-b4d2-7de6ab612bab · outbound

This paper cites Tinto and S.V.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Tinto and S.V

Reference 25

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Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Unresolved cited work

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Observation 3f62752f-ff47-4ff6-a54d-1dda02b06973 · outbound

This paper cites Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Science with the space-based interferometer LISA. V: Extreme mass-ratio inspirals

Reference 27

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Observation 8f690d18-f5d2-4fc8-8ed7-c0e91a626858 · outbound

This paper cites Science with the TianQin observatory: Preliminary result on extreme-mass-ratio inspirals.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Science with the TianQin observatory: Preliminary result on extreme-mass-ratio inspirals

Reference 28

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This paper cites Laser Interferometer Space Antenna.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Laser Interferometer Space Antenna

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Observation f0bbf7c6-9efb-4bc2-a975-ca16e4c7ddcb · outbound

This paper cites Detecting fundamental fields with LISA observations of gravitational waves from extreme mass-ratio inspirals.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Detecting fundamental fields with LISA observations of gravitational waves from extreme mass-ratio inspirals

Reference 30

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Observation f8f9814c-cc29-4a89-ae1f-0335a2071069 · outbound

This paper cites The construction and use of LISA sensitivity curves.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves The construction and use of LISA sensitivity curves

Reference 31

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This paper cites Low-frequency gravitational-wave science with eLISA/NGO.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Low-frequency gravitational-wave science with eLISA/NGO

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This paper cites TianQin: a space-borne gravitational wave detector.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves TianQin: a space-borne gravitational wave detector

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Observation d3aca26e-c4d5-4e82-927c-a65cbff1822f · outbound

This paper cites Science with the TianQin observatory: Preliminary results on stellar-mass binary black holes.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Science with the TianQin observatory: Preliminary results on stellar-mass binary black holes

Reference 34

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This paper cites BBO and the Neutron-Star-Binary Subtraction Problem.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves BBO and the Neutron-Star-Binary Subtraction Problem

Reference 35

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This paper cites Current status of space gravitational wave antenna DECIGO and B-DECIGO.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Current status of space gravitational wave antenna DECIGO and B-DECIGO

Reference 36

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Observation bc51cf6f-a895-4c8e-89bc-d1eceba1ba5f · outbound

This paper cites Ruan, Z.-K.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Ruan, Z.-K

Reference 37

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This paper cites Extreme Mass Ratio Inspirals: LISA's unique probe of black hole gravity.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Extreme Mass Ratio Inspirals: LISA's unique probe of black hole gravity

Reference 38

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This paper cites LISA Capture Sources: Approximate Waveforms, Signal-to-Noise Ratios, and Parameter Estimation Accuracy.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves LISA Capture Sources: Approximate Waveforms, Signal-to-Noise Ratios, and Parameter Estimation Accuracy

Reference 39

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This paper cites "Kludge" gravitational waveforms for a test-body orbiting a Kerr black hole.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves "Kludge" gravitational waveforms for a test-body orbiting a Kerr black hole

Reference 40

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Observation 439f2d75-3200-4282-9c35-dae4188a2eae · outbound

This paper cites Improved analytic extreme-mass-ratio inspiral model for scoping out eLISA data analysis.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Improved analytic extreme-mass-ratio inspiral model for scoping out eLISA data analysis

Reference 41

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Observation d2230f87-5e2f-4e35-9505-d16ed6fe02e9 · outbound

This paper cites The Fast and the Fiducial: Augmented kludge waveforms for detecting extreme-mass-ratio inspirals.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves The Fast and the Fiducial: Augmented kludge waveforms for detecting extreme-mass-ratio inspirals

Reference 42

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Observation 540b72b3-5318-4ed1-b30c-eff62430eb81 · outbound

This paper cites Prospects for determining the nature of the secondaries of extreme mass-ratio inspirals using the spin-induced quadrupole deformation.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Prospects for determining the nature of the secondaries of extreme mass-ratio inspirals using the spin-induced quadrupole deformation

Reference 43

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Observation 7faa2799-e2eb-4f19-9916-313f452a1d63 · outbound

This paper cites Probing astrophysical environment with eccentric extreme mass-ratio inspirals.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Probing astrophysical environment with eccentric extreme mass-ratio inspirals

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Observation a59a31c9-7dd6-402c-9815-a242aa4ab72a · outbound

This paper cites Fast and Fourier: Extreme Mass Ratio Inspiral Waveforms in the Frequency Domain.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Fast and Fourier: Extreme Mass Ratio Inspiral Waveforms in the Frequency Domain

Reference 45

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Observation 03332d30-ced7-4274-9fc3-6ae5073908e5 · outbound

This paper cites Analytic Kludge Waveforms for Extreme Mass Ratio Inspirals of Charged Object around Kerr-Newman Black Hole.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Analytic Kludge Waveforms for Extreme Mass Ratio Inspirals of Charged Object around Kerr-Newman Black Hole

Reference 46

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Observation 5c64a56e-48f5-458d-bb60-d39e7ba11b58 · outbound

This paper cites Probing the Tidal Deformability of the Central Object in an Extreme Mass Ratio Inspiral with Analytic Kludge Waveforms.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Probing the Tidal Deformability of the Central Object in an Extreme Mass Ratio Inspiral with Analytic Kludge Waveforms

Reference 47

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This paper cites FastEMRIWaveforms: New tools for millihertz gravitational-wave data analysis.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves FastEMRIWaveforms: New tools for millihertz gravitational-wave data analysis

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Observation b39ce77c-ebc3-456a-9c9a-bf037f12cd47 · outbound

This paper cites Gravitational waveforms from periodic orbits around a quantum-corrected black hole.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Gravitational waveforms from periodic orbits around a quantum-corrected black hole

Reference 49

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Observation c324d762-d5ba-4381-96c1-0e46183e26fd · outbound

This paper cites Towards adiabatic waveforms for inspiral into Kerr black holes: I. A new model of the source for the time domain perturbation equation.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Towards adiabatic waveforms for inspiral into Kerr black holes: I. A new model of the source for the time domain perturbation equation

Reference 50

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Observation 4463634e-7938-4a92-bbf0-a1f26e414513 · outbound

This paper cites Towards adiabatic waveforms for inspiral into Kerr black holes: II. Dynamical sources and generic orbits.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Towards adiabatic waveforms for inspiral into Kerr black holes: II. Dynamical sources and generic orbits

Reference 51

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Observation 78c0b2b1-4cfa-4e5e-8a59-250b6534c050 · outbound

This paper cites The evolution of circular, non-equatorial orbits of Kerr black holes due to gravitational-wave emission.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves The evolution of circular, non-equatorial orbits of Kerr black holes due to gravitational-wave emission

Reference 52

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Observation 08b4489e-0bbe-46a1-b890-4a4095dff7e6 · outbound

This paper cites Gravitational wave snapshots of generic extreme mass ratio inspirals.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Gravitational wave snapshots of generic extreme mass ratio inspirals

Reference 53

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Observation 1a222451-70db-4a56-b95b-94dcbab5d258 · outbound

This paper cites Gravitational radiation from a particle in circular orbit around a black hole. V. Black-hole absorption and tail corrections.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Gravitational radiation from a particle in circular orbit around a black hole. V. Black-hole absorption and tail corrections

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.650827Z

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Observation 493a4892-a208-4166-be12-082cf6bd82ff · outbound

This paper cites Intermediate and Extreme Mass-Ratio Inspirals -- Astrophysics, Science Applications and Detection using LISA.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Intermediate and Extreme Mass-Ratio Inspirals -- Astrophysics, Science Applications and Detection using LISA

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.655262Z

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Observation 138db6c3-a14c-40f1-b82b-b7969a0f394b · outbound

This paper cites Detecting extreme mass ratio inspiral events in LISA data using the Hierarchical Algorithm for Clusters and Ridges (HACR).

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Detecting extreme mass ratio inspiral events in LISA data using the Hierarchical Algorithm for Clusters and Ridges (HACR)

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.659503Z

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Observation 7d129d42-6251-419a-9b3e-d3bdb51843ed · outbound

This paper cites Improved time-frequency analysis of extreme-mass-ratio inspiral signals in mock LISA data.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Improved time-frequency analysis of extreme-mass-ratio inspiral signals in mock LISA data

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.663449Z

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Observation 50da09d1-4283-45e9-bac9-99259c35e2c4 · outbound

This paper cites Peters, Gravitational Radiation and the Motion of Two Point Masses , Physical Review 136 (1964) 1224.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Peters, Gravitational Radiation and the Motion of Two Point Masses , Physical Review 136 (1964) 1224

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.667603Z

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Observation c09aaffa-018f-43bf-9561-7dfc8cb161f1 · outbound

This paper cites Junker and G.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Junker and G

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.671131Z

Source-reported events for the cited work

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Observation d61933c9-97e9-47b0-a0f1-24d9c488b865 · outbound

This paper cites Eccentric-orbit EMRI gravitational wave energy fluxes to 7PN order.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Eccentric-orbit EMRI gravitational wave energy fluxes to 7PN order

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.674856Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f940fea9-e546-443a-962a-2703e112d4ed · outbound

This paper cites Gravitational waves from inspiralling compact binaries: Angular momentum flux, evolution of the orbital elements and the wave form to the second post-Newtonian order.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Gravitational waves from inspiralling compact binaries: Angular momentum flux, evolution of the orbital elements and the wave form to the second post-Newtonian order

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.679303Z

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Unavailable: canonical work link unavailable.

Observation cd1925a5-1550-4bfe-bae8-b307ca0d1aad · outbound

This paper cites Gopakumar, B.R.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Gopakumar, B.R

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.683517Z

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Observation 824d2da4-d909-4787-8463-786133d970ed · outbound

This paper cites Dynamical Horizons: Energy, Angular Momentum, Fluxes and Balance Laws.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Dynamical Horizons: Energy, Angular Momentum, Fluxes and Balance Laws

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.687387Z

Source-reported events for the cited work

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Observation 1c710967-3d8e-4ae0-a5e9-aa33c6ea2e64 · outbound

This paper cites Hasselmann, On the non-linear energy transfer in a gravity-wave spectru m.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Hasselmann, On the non-linear energy transfer in a gravity-wave spectru m

Reference 64

Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T19:07:27.727349Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 8e4e6de7-1c76-432e-bd22-9b3ffe837970 · outbound

This paper cites Maggiore, Gravitational Waves: Volume 1: Theory and Experiments (2007), 10.1093/acprof:oso/9780198570745.001.0001.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Maggiore, Gravitational Waves: Volume 1: Theory and Experiments (2007), 10.1093/acprof:oso/9780198570745.001.0001

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.696635Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 465572f1-ab4e-4b79-bc26-24dde1f15df0 · outbound

This paper cites Poisson, BOOK REVIEW: Gravitational Waves, Volume 1: Theory and Expe riments, Classical and Quantum Gravity 25 (2008) 209002.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Poisson, BOOK REVIEW: Gravitational Waves, Volume 1: Theory and Expe riments, Classical and Quantum Gravity 25 (2008) 209002

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Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T19:07:27.716054Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 95e73a19-0069-4791-ae8d-bae5bf2b691d · outbound

This paper cites Thorne, Multipole expansions of gravitational radiation , Rev.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Thorne, Multipole expansions of gravitational radiation , Rev

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Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T19:07:27.704885Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation a2010b2b-4048-4369-9fbf-4e3654d1e521 · outbound

This paper cites Gravitational waves from inspiralling compact binaries: Energy flux to third post-Newtonian order.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Gravitational waves from inspiralling compact binaries: Energy flux to third post-Newtonian order

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.707502Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ccbf3e7e-99d7-4118-9d6e-76ad8479771b · outbound

This paper cites Blanchet, B.R.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Blanchet, B.R

Reference 69

Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T19:07:27.693529Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 7a67e562-a05a-46bd-9654-826883c02ccb · outbound

This paper cites High-accuracy numerical simulation of black-hole binaries: Computation of the gravitational-wave energy flux and comparisons with post-Newtonian approximants.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves High-accuracy numerical simulation of black-hole binaries: Computation of the gravitational-wave energy flux and comparisons with post-Newtonian approximants

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.714717Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c73febcb-0d57-4559-9aef-7c3cd24f77d5 · outbound

This paper cites Sensitivity curves for searches for gravitational-wave backgrounds.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Sensitivity curves for searches for gravitational-wave backgrounds

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.718626Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fd9cc7c2-561e-41ba-b56f-76b8b5494034 · outbound

This paper cites Torres and N.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Torres and N

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.722760Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation edc74806-12c2-422e-b5dc-cad519b19749 · outbound

This paper cites Gravitational-wave sensitivity curves.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Gravitational-wave sensitivity curves

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.726547Z

Source-reported events for the cited work

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Observation 5a9613f8-f077-44db-9270-ec92c7285160 · outbound

This paper cites The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.729973Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b896bf8f-35e8-4521-abc1-ed3912a94b94 · outbound

This paper cites The international pulsar timing array project: using pulsars as a gravitational wave detector.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves The international pulsar timing array project: using pulsars as a gravitational wave detector

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Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.733403Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d7155587-a863-4162-9f6d-86879880f8ae · outbound

This paper cites Braun, T.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Braun, T

Reference 76

Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T19:07:27.682692Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation f1f5abf0-8b54-47f9-a3d5-2e7748b1655e · outbound

This paper cites Exploring the Sensitivity of Next Generation Gravitational Wave Detectors.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Exploring the Sensitivity of Next Generation Gravitational Wave Detectors

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Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.740727Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8d321cbc-b0b3-486c-bf54-e4e1b03b4289 · outbound

This paper cites GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run

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Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.744218Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d3db0d56-21f4-4946-b3f2-dd9ffe2f3dff · outbound

This paper cites Tso and the LIGO A+ Collaboration, The A+ upgrade: Improving low-frequency sensitivity in Advanced LIGO , Classical and Quantum Gravity 39 (2022) 155001.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Tso and the LIGO A+ Collaboration, The A+ upgrade: Improving low-frequency sensitivity in Advanced LIGO , Classical and Quantum Gravity 39 (2022) 155001

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Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T19:07:27.671934Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 4c2279c0-d650-47b5-abb5-db95b786da14 · outbound

This paper cites Renormalization group improved black hole spacetimes.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Renormalization group improved black hole spacetimes

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.751740Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6b3855e3-7bcc-473e-a71c-b7a3d7cdbef8 · outbound

This paper cites Planck Stars from a Scale-dependent Gravity theory.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Planck Stars from a Scale-dependent Gravity theory

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.755359Z

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Observation 7aa59a23-2ce7-4672-886e-49e0ee2b6ff6 · outbound

This paper cites Cosmology of the Planck Era from a Renormalization Group for Quantum Gravity.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Cosmology of the Planck Era from a Renormalization Group for Quantum Gravity

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Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.759083Z

Source-reported events for the cited work

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Observation f1622c85-50d9-40d9-858c-7150e548405b · outbound

This paper cites Huang and X.-M.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Huang and X.-M

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Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T19:07:27.661041Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 63f6ea29-39eb-4b41-8b11-2763140b2ab9 · outbound

This paper cites Generalized uncertainty principle and Asymptotic Safe gravity.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Generalized uncertainty principle and Asymptotic Safe gravity

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.766091Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3e1cb335-d868-4421-bdbd-b0412afde3b2 · outbound

This paper cites Analytical solutions of bound timelike geodesic orbits in Kerr spacetime.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Analytical solutions of bound timelike geodesic orbits in Kerr spacetime

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Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.769570Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d8e3c0a0-cc41-4f86-b4dd-f035963e5a0f · outbound

This paper cites Newton, Philosophiae Naturalis Principia Mathematica.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Newton, Philosophiae Naturalis Principia Mathematica

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Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.773205Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6ae8ed4f-e4b2-4b7a-89b2-c54d593c751a · outbound

This paper cites Brouwer and G.M.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Brouwer and G.M

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Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T19:07:27.648866Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation f9f29ab3-1ca0-4108-8871-1d9b66b304e6 · outbound

This paper cites Laskar, A numerical experiment on the chaotic behaviour of the Solar System, Natur.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Laskar, A numerical experiment on the chaotic behaviour of the Solar System, Natur

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Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T19:07:27.636942Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 955aa73a-3b19-4f06-b233-5b3bb6e73d99 · outbound

This paper cites Mayor and D.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Mayor and D

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Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T19:07:27.626370Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation ec9d691c-2b75-4360-bb27-c3cdc3f22ebb · outbound

This paper cites Gravitational waves for eccentric extreme mass ratio inspirals of self-dual spacetime.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Gravitational waves for eccentric extreme mass ratio inspirals of self-dual spacetime

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Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.787146Z

Source-reported events for the cited work

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Observation 7d98af7c-14ba-486d-8309-0e524f5716f5 · outbound

This paper cites Huang, Probing holonomy corrected Schwarzschild black holes with precessing and periodic orbits, Phys.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Huang, Probing holonomy corrected Schwarzschild black holes with precessing and periodic orbits, Phys

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Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T19:07:27.615935Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation f66a8b7c-5a53-4f7d-9737-f2a7f61a3b9a · outbound

This paper cites Lin and X.-M.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Lin and X.-M

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Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T19:07:27.604025Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 57952849-3df4-4c44-ae5b-2e4d5b83eeb4 · outbound

This paper cites Lin and X.-M.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Lin and X.-M

Reference 93

Resolution: verified fuzzy; raw_fallback, observed 2026-08-15T19:07:27.592416Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

Observation 6d2726ed-6111-4288-a3cc-bc00ffc61d97 · outbound

This paper cites A Periodic Table for Black Hole Orbits.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves A Periodic Table for Black Hole Orbits

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Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.801475Z

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Observation aea57d18-f26a-4550-9df0-8bdeb6ef4c26 · outbound

This paper cites Dynamics of Black Hole Pairs I: Periodic Tables.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Dynamics of Black Hole Pairs I: Periodic Tables

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Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.805567Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eaa5c942-7495-415d-a56c-a14f4658788d · outbound

This paper cites Poisson and C.M.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Poisson and C.M

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.809396Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 82bc2aa9-a0d2-4abb-ab89-3620d639d93e · outbound

This paper cites Gravitational Waves from a Compact Star in a Circular, Inspiral Orbit, in the Equatorial Plane of a Massive, Spinning Black Hole, as Observed by LISA.

Distinguishing scale-dependent Planck stars from renormalization group improved Schwarzschild black holes by Gravitational waves Gravitational Waves from a Compact Star in a Circular, Inspiral Orbit, in the Equatorial Plane of a Massive, Spinning Black Hole, as Observed by LISA

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Resolution: unresolved; no resolver link, observed 2026-08-15T19:07:26.813039Z

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