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Paper Citation Record · LEDGER

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes

As of 16 August 2026, this Paper Citation Record lists 35 of 35 outbound references and 0 inbound Pith citation observations for arXiv:1908.07986.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1908.07986 v1

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Reference resolution

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Outbound references

Observation 9771b1d8-b1fd-48cd-a3ac-d48c68574316 · outbound

This paper cites an unresolved cited work.

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes Unresolved cited work

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Observation 22caeaf1-6868-41a4-8906-94d07a17a5c9 · outbound

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Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes Unresolved cited work

Reference 2

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This paper cites However, this state corresponds to pure incompressible fluids [14].

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes However, this state corresponds to pure incompressible fluids [14]

Reference 3

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Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes Unresolved cited work

Reference 4

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Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes Unresolved cited work

Reference 5

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This paper cites Here, the TOV-equation is solved for the pressure starting from a given P (r = 0) =P0 up to a radius, where the pressure vanishes.

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes Here, the TOV-equation is solved for the pressure starting from a given P (r = 0) =P0 up to a radius, where the pressure vanishes

Reference 6

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This paper cites The total mass of the core is calculated through the integra- tion: mtot(r =Rcore) = ∫ Rcore 0 (εb +εφ)dr.

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes The total mass of the core is calculated through the integra- tion: mtot(r =Rcore) = ∫ Rcore 0 (εb +εφ)dr

Reference 7

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This paper cites and MSuSu ≈ MSchw.

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes and MSuSu ≈ MSchw

Reference 8

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Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes Unresolved cited work

Reference 9

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This paper cites The values at τage = 1000, 10000 yrs and τage = 10 Myr are chosen to enable partial comparison with observations of the glitch events of Vela and Crab pulsars.

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes The values at τage = 1000, 10000 yrs and τage = 10 Myr are chosen to enable partial comparison with observations of the glitch events of Vela and Crab pulsars

Reference 10

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This paper cites (2007), Progress in Particle and Nuclear Physics, 351, 58.

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes (2007), Progress in Particle and Nuclear Physics, 351, 58

Reference 11

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Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes Unresolved cited work

Reference 12

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Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes & Yakovlev, D.G

Reference 13

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Observation d5bb80cb-e333-49fe-b41f-8ca46840c461 · outbound

This paper cites (2011) MNRAS, 414, 1679.

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes (2011) MNRAS, 414, 1679

Reference 14

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This paper cites (2014) Int.

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes (2014) Int

Reference 15

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Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes Unresolved cited work

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This paper cites (2007), Compact Objects in Astrophysics, Springer, Heidelberg.

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes (2007), Compact Objects in Astrophysics, Springer, Heidelberg

Reference 17

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This paper cites (2007), Special and General Relativity.

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes (2007), Special and General Relativity

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Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes Unresolved cited work

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This paper cites (1979) , Phys.

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes (1979) , Phys

Reference 20

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This paper cites (1999) A&A, 344, 151.

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes (1999) A&A, 344, 151

Reference 21

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This paper cites (2007), Phys Rev Lett 99(26):265302.

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes (2007), Phys Rev Lett 99(26):265302

Reference 22

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This paper cites (1994) ApJ Letters, 423, L117.

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes (1994) ApJ Letters, 423, L117

Reference 23

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Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes 1” corresponds to the low “Z

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This paper cites (1984) Physical Review D, Volu.

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes (1984) Physical Review D, Volu

Reference 25

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Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes Unresolved cited work

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This paper cites (2018), Journal of Modern Physics, 9, 70-83.

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes (2018), Journal of Modern Physics, 9, 70-83

Reference 27

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This paper cites (2012) MNRAS, 423.2893.

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes (2012) MNRAS, 423.2893

Reference 28

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This paper cites (2018), Journal of Modern Physics, 9, 4, jmp.2018.94038.

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes (2018), Journal of Modern Physics, 9, 4, jmp.2018.94038

Reference 29

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This paper cites (2018), Journal of Modern Physics, 9, 4, jmp.2018.94037.

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes (2018), Journal of Modern Physics, 9, 4, jmp.2018.94037

Reference 30

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Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes & Yunes, N., (2019) ”The new frontier of gravitational waves”

Reference 31

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Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes Unresolved cited work

Reference 32

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Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes & Freire, P

Reference 33

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Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes Unresolved cited work

Reference 34

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Observation a8bc6374-fd03-4d6d-94f0-0b9257c4e210 · outbound

This paper cites an unresolved cited work.

Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes Unresolved cited work

Reference 35

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unresolved
raw_fallback, observed 2026-08-14T11:58:03.151981Z

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source=pdf_text observed=2026-08-14T11:58:02.676689Z digest=sha256:6844a12ef914c803c2e891e359c9a487776075b3fce41f56120af00bcba0c76b

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