From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data | Paper Citation Record

Observation 55e0806d-f2d7-4a3e-9594-9b6c41f796bf · outbound

This paper cites [16]): One model pa- rameter (Gµ, the string tension in units of Newton’ s constant), GW emission from cusps and kinks [83–85].

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data [16]): One model pa- rameter (Gµ, the string tension in units of Newton’ s constant), GW emission from cusps and kinks [83–85]

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:07.279242Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a38de394-abc3-43d3-aa7e-a3dd0565575b · outbound

This paper cites [16]): Two model parameters ( Gµ and pκ, the decay parameter con- trolling the lifetime of the string network), GW emis- sion from cusps on loops and from segments [66].

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data [16]): Two model parameters ( Gµ and pκ, the decay parameter con- trolling the lifetime of the string network), GW emis- sion from cusps on loops and from segments [66]

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:07.376535Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 97a8cb39-f6d2-4546-85e4-efdc2ac563ac · outbound

This paper cites slow-roll.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data slow-roll

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:07.495342Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fc4035ef-dd75-4c9c-aafe-a4ab81426ac1 · outbound

This paper cites The Nanohertz Gravitational Wave Astronomer.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data The Nanohertz Gravitational Wave Astronomer

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:07.607861Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1d365b56-6f68-4002-938f-0aaa5fe435cd · outbound

This paper cites Pulsar timing and polarimetry: results and perspectives.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Pulsar timing and polarimetry: results and perspectives

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:07.704411Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bee6722e-d8c7-42b3-87c2-b7c6a8879a66 · outbound

This paper cites Pulsar Timing Arrays.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Pulsar Timing Arrays

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:07.825405Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c23dd4b2-4605-4ada-ab44-5543aee96b48 · outbound

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

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:07.950602Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7feb6fc7-9ace-4f74-9f0b-582f91541efa · outbound

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

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:08.049232Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1d019c36-1b34-41ea-8a0c-c167c7f14cda · outbound

This paper cites Search for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Search for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:08.106063Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0cb200a5-cedd-435c-ba9c-b6e6c6b41049 · outbound

This paper cites Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:08.215173Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e2890a6f-195d-41df-933f-f0f6a88743ee · outbound

This paper cites Comparing recent PTA results on the nanohertz stochastic gravitational wave background.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Comparing recent PTA results on the nanohertz stochastic gravitational wave background

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:08.342941Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 53abd840-e9bb-467f-b8f7-9e2c2e3e9738 · outbound

This paper cites The MeerKAT Pulsar Timing Array: The first search for gravitational waves with the MeerKAT radio telescope.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data The MeerKAT Pulsar Timing Array: The first search for gravitational waves with the MeerKAT radio telescope

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:08.429931Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3df09fca-c1ac-41f9-b673-7321b56bb904 · outbound

This paper cites Hellings and G.s.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Hellings and G.s

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:08.476847Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6e8b62b6-ea03-4b4e-9eff-6f736dfdf20c · outbound

This paper cites Answers to frequently asked questions about the pulsar timing array Hellings and Downs curve.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Answers to frequently asked questions about the pulsar timing array Hellings and Downs curve

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:08.543614Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4a4cc6d5-c1ea-435f-a74e-4a906a525bce · outbound

This paper cites Astrophysics Milestones For Pulsar Timing Array Gravitational Wave Detection.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Astrophysics Milestones For Pulsar Timing Array Gravitational Wave Detection

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:08.643248Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a9778fd7-efed-451d-a9a6-52bdd19ea6a6 · outbound

This paper cites The NANOGrav 15-year Data Set: Constraints on Supermassive Black Hole Binaries from the Gravitational Wave Background.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data The NANOGrav 15-year Data Set: Constraints on Supermassive Black Hole Binaries from the Gravitational Wave Background

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:08.725085Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e0caff85-cf36-4746-9f9d-c072336a788e · outbound

This paper cites Gravitational Waves from SMBH Binaries in Light of the NANOGrav 15-Year Data.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Gravitational Waves from SMBH Binaries in Light of the NANOGrav 15-Year Data

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:08.769855Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d81ffe99-b1ea-43af-b811-9d0750e35c61 · outbound

This paper cites an unresolved cited work.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Unresolved cited work

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:08.828404Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ea6905d9-0cb4-4368-a32a-aab203bba1c3 · outbound

This paper cites The NANOGrav 15-year Data Set: Search for Signals from New Physics.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data The NANOGrav 15-year Data Set: Search for Signals from New Physics

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:08.926672Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 041b41a4-aa97-4ea7-a390-c9ea00f5bafc · outbound

This paper cites The second data release from the European Pulsar Timing Array: IV. Implications for massive black holes, dark matter and the early Universe.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data The second data release from the European Pulsar Timing Array: IV. Implications for massive black holes, dark matter and the early Universe

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:08.992790Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b5a4dd0c-0bfa-4514-99e0-75a7060628a8 · outbound

This paper cites Cosmological Background Interpretation of Pulsar Timing Array Data.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Cosmological Background Interpretation of Pulsar Timing Array Data

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:09.074914Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 577c8a4c-8d08-4cc0-8ddc-65ed6c685be6 · outbound

This paper cites What is the source of the PTA GW signal?.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data What is the source of the PTA GW signal?

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:09.165813Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 324b4579-8c42-4a91-8dc7-dcd32b6717ae · outbound

This paper cites Gravitational Wave Experiments and Early Universe Cosmology.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Gravitational Wave Experiments and Early Universe Cosmology

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:09.237970Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dd008679-2527-4c9e-9848-33c3d3351382 · outbound

This paper cites Cosmological Backgrounds of Gravitational Waves.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Cosmological Backgrounds of Gravitational Waves

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:09.346963Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a9d4c0f5-42fc-4e90-b4f2-41debf13307d · outbound

This paper cites Inflationary interpretation of the stochastic gravitational wave background signal detected by pulsar timing array experiments.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Inflationary interpretation of the stochastic gravitational wave background signal detected by pulsar timing array experiments

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:09.508593Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 52fca3d5-079b-43ba-93f4-9878173f1347 · outbound

This paper cites Broken blue-tilted inflationary gravitational waves: a joint analysis of NANOGrav 15-year and BICEP/Keck 2018 data.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Broken blue-tilted inflationary gravitational waves: a joint analysis of NANOGrav 15-year and BICEP/Keck 2018 data

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:09.596210Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4aa47a0b-3799-43da-8a01-2cd8f734435e · outbound

This paper cites Single field inflation in the light of Pulsar Timing Array Data: Quintessential interpretation of blue tilted tensor spectrum through Non-Bunch Davies initial condition.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Single field inflation in the light of Pulsar Timing Array Data: Quintessential interpretation of blue tilted tensor spectrum through Non-Bunch Davies initial condition

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:09.697102Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8b5e2300-1161-4adf-b975-efc04d9e23f1 · outbound

This paper cites The recent gravitational wave observation by pulsar timing arrays and primordial black holes: the importance of non-gaussianities.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data The recent gravitational wave observation by pulsar timing arrays and primordial black holes: the importance of non-gaussianities

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:09.739887Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ea6f1b96-4e03-4577-826a-bb93b91e06d7 · outbound

This paper cites Limits on scalar-induced gravitational waves from the stochastic background by pulsar timing array observations.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Limits on scalar-induced gravitational waves from the stochastic background by pulsar timing array observations

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:09.787434Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation be41dc57-1519-43cd-9c20-90b7b9012710 · outbound

This paper cites The Detected Stochastic Gravitational Waves and Subsolar-Mass Primordial Black Holes.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data The Detected Stochastic Gravitational Waves and Subsolar-Mass Primordial Black Holes

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:09.842152Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 693b7845-7ded-49ed-8333-d26f9832b043 · outbound

This paper cites Implications of Pulsar Timing Array Data for Scalar-Induced Gravitational Waves and Primordial Black Holes: Primordial Non-Gaussianity $f_{\mathrm{NL}}$ Considered.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Implications of Pulsar Timing Array Data for Scalar-Induced Gravitational Waves and Primordial Black Holes: Primordial Non-Gaussianity $f_{\mathrm{NL}}$ Considered

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:09.915604Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b3e20651-e616-4773-bf44-78d7482a5f5f · outbound

This paper cites Induced Gravitational Waves from Ultra Slow-Roll Inflation and Pulsar Timing Arrays Observations.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Induced Gravitational Waves from Ultra Slow-Roll Inflation and Pulsar Timing Arrays Observations

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:10.019871Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e5a9996e-ae32-4459-8841-480956ce1701 · outbound

This paper cites Implications for the non-Gaussianity of curvature perturbation from pulsar timing arrays.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Implications for the non-Gaussianity of curvature perturbation from pulsar timing arrays

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:10.119555Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ea8c30a4-d012-45f6-9f75-f0093415d3a7 · outbound

This paper cites Scalar-induced gravitational wave interpretation of PTA data: the role of scalar fluctuation propagation speed.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Scalar-induced gravitational wave interpretation of PTA data: the role of scalar fluctuation propagation speed

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:10.235820Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9c52e7e7-1b46-4559-8b08-bd6273ffc962 · outbound

This paper cites Curbing PBHs with PTAs.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Curbing PBHs with PTAs

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:10.340438Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b92281bd-156d-4cda-993f-a032ee6f3b69 · outbound

This paper cites Footprints of the QCD Crossover on Cosmological Gravitational Waves at Pulsar Timing Arrays.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Footprints of the QCD Crossover on Cosmological Gravitational Waves at Pulsar Timing Arrays

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:10.499633Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 531ec7c1-deb1-47b7-90f5-c5af9971529a · outbound

This paper cites Have pulsar timing array methods detected a cosmological phase transition?.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Have pulsar timing array methods detected a cosmological phase transition?

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:10.657440Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ffccb723-2323-42cf-9c7b-be1eaab06a08 · outbound

This paper cites QCD-Collapsed Domain Walls: QCD Phase Transition and Gravitational Wave Spectroscopy.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data QCD-Collapsed Domain Walls: QCD Phase Transition and Gravitational Wave Spectroscopy

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:10.769302Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eb14b344-66b4-42c4-ada1-ff0686316bec · outbound

This paper cites Self-interacting dark matter implied by nano-Hertz gravitational waves.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Self-interacting dark matter implied by nano-Hertz gravitational waves

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:10.842289Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d262da59-7d2b-46e5-903f-21aad4402672 · outbound

This paper cites Pulsar Timing Array Stochastic Background from light Kaluza-Klein resonances.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Pulsar Timing Array Stochastic Background from light Kaluza-Klein resonances

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:10.951427Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ae55f041-f2df-4884-a153-a1190705495e · outbound

This paper cites Did we hear the sound of the Universe boiling? Analysis using the full fluid velocity profiles and NANOGrav 15-year data.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Did we hear the sound of the Universe boiling? Analysis using the full fluid velocity profiles and NANOGrav 15-year data

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:11.063763Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 74b6ce29-e325-461c-85d3-2ae23f73f945 · outbound

This paper cites A collider test of nano-Hertz gravitational waves from pulsar timing arrays.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data A collider test of nano-Hertz gravitational waves from pulsar timing arrays

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:11.172855Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4a47e78e-f113-4738-b98c-bf1b4ee96c1d · outbound

This paper cites The split majoron model confronts the NANOGrav signal and cosmological tensions.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data The split majoron model confronts the NANOGrav signal and cosmological tensions

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:11.243503Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a3da7c26-4429-4472-b724-ce4b52193f87 · outbound

This paper cites First-order Phase Transition interpretation of PTA signal produces solar-mass Black Holes.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data First-order Phase Transition interpretation of PTA signal produces solar-mass Black Holes

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:11.314901Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ec03dbb5-0416-4904-8074-7cb7e6494963 · outbound

This paper cites an unresolved cited work.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Unresolved cited work

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:11.424472Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c50f2f76-76ce-499b-a894-92b48e4d28b2 · outbound

This paper cites Cosmic Superstrings Revisited in Light of NANOGrav 15-Year Data.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Cosmic Superstrings Revisited in Light of NANOGrav 15-Year Data

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:11.529495Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e39b3e2c-13a7-4141-96d2-77c9fb84eb7c · outbound

This paper cites The nanohertz stochastic gravitational wave background from cosmic string loops and the abundant high redshift massive galaxies.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data The nanohertz stochastic gravitational wave background from cosmic string loops and the abundant high redshift massive galaxies

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:11.670352Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e22bf8c3-23e0-47f0-92da-c2cb34f21316 · outbound

This paper cites Superheavy quasi-stable strings and walls bounded by strings in the light of NANOGrav 15 year data.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Superheavy quasi-stable strings and walls bounded by strings in the light of NANOGrav 15 year data

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:11.773940Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ed46550e-ec83-49a8-8078-79a5f6b093ec · outbound

This paper cites Dark energy, D-branes, and Pulsar Timing Arrays.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Dark energy, D-branes, and Pulsar Timing Arrays

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:11.871043Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cf0b0420-e13a-42bb-ac6d-f061c7e0869f · outbound

This paper cites Constraining Postinflationary Axions with Pulsar Timing Arrays.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Constraining Postinflationary Axions with Pulsar Timing Arrays

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:11.920578Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6e29461a-e3be-46b2-b31a-7325d2ffe77e · outbound

This paper cites Singling out SO(10) GUT models using recent PTA results.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Singling out SO(10) GUT models using recent PTA results

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:12.002259Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f63ac9df-afc7-4615-95e8-a96261070f43 · outbound

This paper cites Stochastic gravitational wave background: birth from string-wall death.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Stochastic gravitational wave background: birth from string-wall death

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:12.088475Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 485db518-960a-4cb2-9d39-5b700c1e8ee3 · outbound

This paper cites Gravitational wave signatures of no-scale Supergravity in NANOGrav and beyond.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Gravitational wave signatures of no-scale Supergravity in NANOGrav and beyond

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:12.143633Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cc3a6637-baca-42de-8352-dc433158e0da · outbound

This paper cites Gravitational Waves from Domain Wall Collapse, and Application to Nanohertz Signals with QCD-coupled Axions.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Gravitational Waves from Domain Wall Collapse, and Application to Nanohertz Signals with QCD-coupled Axions

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:12.195621Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d77973a6-7bcf-4629-8a73-60c3b5f2ddf2 · outbound

This paper cites Footprints of Axion-Like Particle in Pulsar Timing Array Data and James Webb Space Telescope Observations.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Footprints of Axion-Like Particle in Pulsar Timing Array Data and James Webb Space Telescope Observations

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:12.267565Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 894fff8c-cc7e-4868-b1f0-82eb33a4cbaf · outbound

This paper cites Axionic domain walls at Pulsar Timing Arrays: QCD bias and particle friction.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Axionic domain walls at Pulsar Timing Arrays: QCD bias and particle friction

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:12.378894Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5f6cdac4-826b-4133-b6a2-c19228cfee61 · outbound

This paper cites Domain wall interpretation of the PTA signal confronting black hole overproduction.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Domain wall interpretation of the PTA signal confronting black hole overproduction

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:12.544986Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 167b554d-b248-4b66-8806-039fec46f752 · outbound

This paper cites Clockwork axion footprint on nano-hertz stochastic gravitational wave background.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Clockwork axion footprint on nano-hertz stochastic gravitational wave background

Reference 58

Resolution: verified exact; local_arxiv, observed 2026-08-06T21:42:19.041230Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 7bcf20ec-98fe-4b16-8d7f-50d4e11241b9 · outbound

This paper cites NANOGrav spectral index $\gamma=3$ from melting domain walls.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data NANOGrav spectral index $\gamma=3$ from melting domain walls

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:12.746766Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cd9b5a5a-2fc6-4ce6-9463-d3cd1a028f45 · outbound

This paper cites The NANOGrav 15-year Data Set: Search for Anisotropy in the Gravitational-Wave Background.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data The NANOGrav 15-year Data Set: Search for Anisotropy in the Gravitational-Wave Background

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:12.913850Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 74f3343d-cf13-4274-b509-d41c6e3d6794 · outbound

This paper cites Beyond the Background: Gravitational Wave Anisotropy and Continuous Waves from Supermassive Black Hole Binaries.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Beyond the Background: Gravitational Wave Anisotropy and Continuous Waves from Supermassive Black Hole Binaries

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:13.102380Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e2945bb1-03e5-414e-9296-9527969cc981 · outbound

This paper cites Pulsar timing array sensitivity to anisotropies in the gravitational wave background.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Pulsar timing array sensitivity to anisotropies in the gravitational wave background

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:13.290386Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8db50715-f3a4-4d79-ba7a-2988730b6bcf · outbound

This paper cites The impact of cosmic variance on PTAs anisotropy searches.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data The impact of cosmic variance on PTAs anisotropy searches

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:13.428114Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b2b9c601-2545-4e95-a780-808544a3a619 · outbound

This paper cites The NANOGrav 15-year Data Set: Bayesian Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data The NANOGrav 15-year Data Set: Bayesian Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:13.579076Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 94578063-bb8a-441f-b171-7a3ab013594a · outbound

This paper cites The NANOGrav 12.5-year data set: A computationally efficient eccentric binary search pipeline and constraints on an eccentric supermassive binary candidate in 3C 66B.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data The NANOGrav 12.5-year data set: A computationally efficient eccentric binary search pipeline and constraints on an eccentric supermassive binary candidate in 3C 66B

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:13.734857Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4336dd19-f1dd-4ccf-9ad7-4d81fdb3ed50 · outbound

This paper cites Observational Signatures of Supermassive Black Hole Binaries.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Observational Signatures of Supermassive Black Hole Binaries

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:13.924220Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 14932d9f-a834-4de6-8043-824305e143ce · outbound

This paper cites Sousa, Cosmic strings and gravitational waves, Gen.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Sousa, Cosmic strings and gravitational waves, Gen

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:14.072532Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2c284551-9d49-431d-b503-d83b39481b8a · outbound

This paper cites Schmitz and T.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Schmitz and T

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:14.196573Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation aa7e4e5c-d524-4694-b7a2-5a1fc83ade59 · outbound

This paper cites Stochastic gravitational-wave background from metastable cosmic strings.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Stochastic gravitational-wave background from metastable cosmic strings

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:14.368954Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bc1a20b4-3668-4869-acbd-539dfd0f2903 · outbound

This paper cites Metastable cosmic strings.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Metastable cosmic strings

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:14.539642Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e9c5ce04-2d50-4bb4-919d-bc3ad7f77985 · outbound

This paper cites Scalar induced gravitational waves review.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Scalar induced gravitational waves review

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:14.670083Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6f4a54cb-86bf-4d7a-8aac-eb7a78a3c807 · outbound

This paper cites The Need For Speed: Rapid Refitting Techniques for Bayesian Spectral Characterization of the Gravitational Wave Background Using PTAs.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data The Need For Speed: Rapid Refitting Techniques for Bayesian Spectral Characterization of the Gravitational Wave Background Using PTAs

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:14.819941Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 70d9e3b1-b33a-4486-9c45-3d30aa833d0c · outbound

This paper cites ENTERPRISE: Enhanced Numerical Toolbox Enabling a Robust PulsaR Inference SuitE.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data ENTERPRISE: Enhanced Numerical Toolbox Enabling a Robust PulsaR Inference SuitE

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:14.990587Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 980f245f-7e2b-414d-9893-cc3be50c0bf9 · outbound

This paper cites Taylor, P .T.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Taylor, P .T

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:15.116278Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 42c4d565-0b72-4637-89f2-e090afd4c754 · outbound

This paper cites PTArcade.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data PTArcade

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:15.266947Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8099eb3f-820c-47ea-a598-0ba0979d67d9 · outbound

This paper cites Maggiore, Gravitational Waves.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Maggiore, Gravitational Waves

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:15.400787Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7c5a935d-f155-4443-974c-af9d84509cdd · outbound

This paper cites Maggiore, Gravitational Waves.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Maggiore, Gravitational Waves

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:15.523608Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e189b102-3a67-4c76-82d5-eba49ea05eb3 · outbound

This paper cites 10.5281/zenodo.8092346.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data 10.5281/zenodo.8092346

Reference 78

Resolution: verified exact; doi, observed 2026-08-06T21:42:18.215352Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 34b040d6-1163-4308-8614-b123e9e8580a · outbound

This paper cites The NANOGrav 15 yr Data Set: Running of the Spectral Index.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data The NANOGrav 15 yr Data Set: Running of the Spectral Index

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:15.887082Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 603793d1-a122-4f8e-8f36-aec8121f24a0 · outbound

This paper cites Realistic sensitivity curves for pulsar timing arrays.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Realistic sensitivity curves for pulsar timing arrays

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:16.138115Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ce4ec2d8-5fe8-4fc4-9de7-84a02b394afa · outbound

This paper cites New Sensitivity Curves for Gravitational-Wave Signals from Cosmological Phase Transitions.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data New Sensitivity Curves for Gravitational-Wave Signals from Cosmological Phase Transitions

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:16.329778Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c91ad59f-979d-4397-98be-2ca2af9a1872 · outbound

This paper cites Probing the Universe through the Stochastic Gravitational Wave Background.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Probing the Universe through the Stochastic Gravitational Wave Background

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:16.568372Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0a35a832-de8b-4820-ab96-b55cf99f94a4 · outbound

This paper cites Using a Primordial Gravitational Wave Background to Illuminate New Physics.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Using a Primordial Gravitational Wave Background to Illuminate New Physics

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:16.799126Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 04809225-84bb-4423-b8d9-8507148b9928 · outbound

This paper cites Imprint of a scalar era on the primordial spectrum of gravitational waves.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Imprint of a scalar era on the primordial spectrum of gravitational waves

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:16.978603Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 879d1513-9a74-4ab1-bca3-029af8a1c7df · outbound

This paper cites Gravitational waves from first-order phase transitions in LISA: reconstruction pipeline and physics interpretation.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Gravitational waves from first-order phase transitions in LISA: reconstruction pipeline and physics interpretation

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:17.176480Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 735b0c30-fac4-4754-89da-0483eeb4960a · outbound

This paper cites Large parallel cosmic string simulations: New results on loop production.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Large parallel cosmic string simulations: New results on loop production

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:17.267465Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0edfb344-aa2b-4064-8091-a4772a1a56d6 · outbound

This paper cites The number of cosmic string loops.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data The number of cosmic string loops

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:17.340149Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0e8689e2-a8bf-4ac6-a428-e1a15a76e273 · outbound

This paper cites Stochastic gravitational wave background from smoothed cosmic string loops.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Stochastic gravitational wave background from smoothed cosmic string loops

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:17.483393Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4e0da041-e135-44e0-bc16-b4d655392e43 · outbound

This paper cites Gravitational Waves Induced by Scalar Perturbations with a Lognormal Peak.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Gravitational Waves Induced by Scalar Perturbations with a Lognormal Peak

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:17.617310Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d8ce301e-a2df-4a4c-aea0-7a132c327714 · outbound

This paper cites Semianalytic Calculation of Gravitational Wave Spectrum Nonlinearly Induced from Primordial Curvature Perturbations.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Semianalytic Calculation of Gravitational Wave Spectrum Nonlinearly Induced from Primordial Curvature Perturbations

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:17.714193Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eacc3d51-eef7-4912-908c-5e01663fa414 · outbound

This paper cites A Cosmological Signature of the SM Higgs Instability: Gravitational Waves.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data A Cosmological Signature of the SM Higgs Instability: Gravitational Waves

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:17.769620Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 65c5727a-023b-402c-a1e4-d5a3abd6ef9c · outbound

This paper cites Planck 2018 results. X. Constraints on inflation.

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data Planck 2018 results. X. Constraints on inflation

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-06T21:42:17.902495Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Coverage vector

Reference resolution

Outbound references

Pith citing papers