Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-01T04:04:30.099432Z
Paper Citation Record · LEDGER
As of 16 August 2026, this Paper Citation Record lists 40 of 40 outbound references and 0 inbound Pith citation observations for arXiv:2607.22977.
A citation records a reference. It does not transfer a finding from one paper to another.
Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-01T04:04:30.099432Z
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links
A source-named dated measurement, never combined with another source.
Source: cited_works
40 of 40 outbound references displayed
External citation measurements
No source-named external measurement is stored.
Observation 9870551e-03b6-4be4-be6a-5f180ff0041a · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unresolved cited work
Reference 1
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Observation f51cfe1c-c9f3-425f-b78b-adc20c7badba · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unresolved cited work
Reference 2
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Observation 9b7e8469-d58a-4d8a-b19e-9e4725515504 · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions For instance, ifβ= 9 50m2, the extremal charge is exactlyQext = 2 √ 5 3 m, which results in a single degenerate event horizon located atr+ = 5 3m
Reference 3
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Observation 7250ebd2-0ddf-43fb-a3a2-e3604d5270c8 · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unresolved cited work
Reference 4
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Observation b62c011c-0fe5-4ac2-bd57-af9e241123b6 · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unresolved cited work
Reference 5
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Observation de9855e0-1dc7-4933-8d09-e9ea54fe4e44 · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unresolved cited work
Reference 6
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Observation ee961f77-658f-47d3-9f3f-c9ea3cf4e1ea · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions ξ=0 ξ=0.05/m3 ξ=0.1/m3 ξ=0.16/m3 0 2 4 6 8 10 -1.0 -0.5 0.0 0.5 1.0 1.5 r/m Δr Σ 1.8 1.9 2.0 2.1 2.2 -0.2 -0.1 0.0 0.1 0.2 (b)a= 0, n= 0.3mandQ e = 0.5m
Reference 7
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Observation a8b0900f-b23f-404a-a2dd-c8d83fae02a0 · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Similarly, forQe = 0.5mandξ∈[0,0.16], the horizon grows withξ, and is larger than in the non-rotating case
Reference 8
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Observation f1991ca4-c586-4cdf-90be-55a5a3a1c876 · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Additionally, the energy density should not be exceeded by anypressure, such thatµ+pα≥0, α= 1,2,3
Reference 9
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Observation faa2dfd0-ab0b-4f50-b75e-1b2a6009eb95 · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions This leads to the following inequalities for the Cubic NLED-KN-NUT-Λ, 0≤(µ−p 1,2) =− Tµ µ 2 = (Q2 e +Q 2 m) 4πΣ (1 +βn 2)(1 +βn 2−3r 2β)β
Reference 10
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Observation 98dc5a67-0fa8-4d06-a32a-66273ea1277a · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions In terms of theOTab components, SEC amounts toµ+p 1 +p 2 +p 3≥0
Reference 11
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Observation 82f70561-8f55-47b9-bc61-b325657b45ae · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unresolved cited work
Reference 12
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Observation 2e33f697-3796-4cbe-b8b5-b9739b8baf94 · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unresolved cited work
Reference 13
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Observation b35df100-a7f4-4396-80a2-4cdd7cfbc41a · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Quantum Frontiers
Reference 14
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Observation ecc1a431-bd17-4943-9bc6-295dd7902205 · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Equivalently, one may attempt to reconstruct L(E,B)from the constitutive relationsD= ∂L ∂E andH=− ∂L ∂B by solving the corresponding differential equation for L(E,B)
Reference 15
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Observation 420aa6b5-83ff-4256-8166-68bd8e01ed0a · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unresolved cited work
Reference 16
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Observation b5a378c7-e19c-41e2-a9b3-cd65024715d9 · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unresolved cited work
Reference 17
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Observation c4c0dc5f-2cf1-4e93-af13-ba1b51437d36 · outbound
Reference 18
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Observation 293585ac-20be-4e07-a17c-149e62819683 · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unresolved cited work
Reference 19
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Observation 78a335f4-806b-428f-a229-82f14b22f333 · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unresolved cited work
Reference 20
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Observation 3bcd5234-3207-4d7e-a02a-62cf5b83d5e0 · outbound
Reference 21
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Observation 94c15f48-a3fd-4e83-ae23-7d5c15c727aa · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unresolved cited work
Reference 22
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Observation 06b5f8c0-c7e6-48b9-9069-1e6497e82de1 · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unresolved cited work
Reference 23
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Observation a2b763a2-00e8-46de-85a3-3fd32c91c18e · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Alencar, Albert Duran-Cabacés, Diego Rubiera-Garcia, and Diego Sáez-Chillón Gómez
Reference 24
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Observation 09a2bc9a-5412-4aa3-8114-91d31b89a7b3 · outbound
Reference 25
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Observation f7eebcde-da98-4507-a338-0c1f26ba3b80 · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Nonlinear electromagnetic generalization of the Kerr-Newman solution with cosmological constant
Reference 26
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Observation 4075afdd-4d25-43a7-a391-39c8e1930bdf · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unresolved cited work
Reference 27
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Observation fda46736-ef35-46e9-9b4f-e1b32a3748a3 · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Kubizňák and P
Reference 28
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Observation a6767fb2-b7d7-4b5f-afbc-db15be990fe4 · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Breton and C
Reference 29
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Observation 7eccb0bf-70a2-401d-9b88-f7282b026ec8 · outbound
Reference 30
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Observation 717f891d-4183-4306-998f-97708b34d1ea · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unresolved cited work
Reference 31
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Observation 4bc54ba8-1939-4b66-bbcd-031ce52b2fb6 · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unresolved cited work
Reference 32
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Observation ed4bff7a-9a89-4f06-8ab2-63888fe3026f · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unresolved cited work
Reference 33
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Observation 01938221-8cb9-4f81-aada-15885a033af6 · outbound
Reference 34
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Observation cf48d4b6-b8cd-49d2-b790-fb15c8866bc5 · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unveilingtheelectrodynamicsofthefirstnonlinearlychargedrotatingblackhole.Annals Phys., 469:169771,
Reference 35
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Observation 7a751b90-f157-4784-964a-f3e00d02f26a · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Grenzebach, V
Reference 37
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Observation 1aa111dc-9c35-4c96-b94a-6f4115c6dbf4 · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unresolved cited work
Reference 38
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Observation 8b6688fb-8f2a-4f97-89d7-9340d2eff6d3 · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Hackmann and C
Reference 39
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Observation b5a0065e-4f4a-41d1-a023-1afd25588cfc · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unresolved cited work
Reference 40
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Observation e4453546-1ca0-4414-94e7-68682c32046d · outbound
Nonlinear electrodynamics in Kerr-Newman-NUT-$\Lambda$ spacetime: exact solutions, horizons, and energy conditions Unveiling the electrodynamics of the first nonlinearly charged rotating black hole
Reference 2024
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No inbound Pith citation observations are available.