Charged cosmological black holes: a thorough study of a family of solutions | Paper Citation Record

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This paper cites (14), we ﬁnd the same solution for the potential as in [29],i.e., (dV dφ )2 = 3µ4V , (34) V = 3µ4 4 (φ−V0)2 , (35) and it is then seen that the entire system is consistent.

Charged cosmological black holes: a thorough study of a family of solutions (14), we ﬁnd the same solution for the potential as in [29],i.e., (dV dφ )2 = 3µ4V , (34) V = 3µ4 4 (φ−V0)2 , (35) and it is then seen that the entire system is consistent

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This paper cites Hence, considering that the isotropic coordinate is real, the domain of the areal radius coordi- nateR should be restricted to the intervalsR+≤R< ∞ and 0≤R≤R−.

Charged cosmological black holes: a thorough study of a family of solutions Hence, considering that the isotropic coordinate is real, the domain of the areal radius coordi- nateR should be restricted to the intervalsR+≤R< ∞ and 0≤R≤R−

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This paper cites We then conclude that, form2 =q2, theisotropiccoordinate r covers(once) all the range ofR.

Charged cosmological black holes: a thorough study of a family of solutions We then conclude that, form2 =q2, theisotropiccoordinate r covers(once) all the range ofR

Reference 3

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This paper cites Therefore, form2 <q 2, the isotropic coordinate r covers (twice) all the range ofR.

Charged cosmological black holes: a thorough study of a family of solutions Therefore, form2 <q 2, the isotropic coordinate r covers (twice) all the range ofR

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Observation 36660726-d1e7-4113-b52f-426e5f303ea6 · outbound

This paper cites (36) and (39)] for which the a(t)r→ 0 limit corresponds toR→∞ , whileR = 0 cor- responds to a(t)r = (−m±|q|)/2, where the isotropic coordinater is allowed to assume negative values.

Charged cosmological black holes: a thorough study of a family of solutions (36) and (39)] for which the a(t)r→ 0 limit corresponds toR→∞ , whileR = 0 cor- responds to a(t)r = (−m±|q|)/2, where the isotropic coordinater is allowed to assume negative values

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This paper cites First of all, Eq.

Charged cosmological black holes: a thorough study of a family of solutions First of all, Eq

Reference 6

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This paper cites The spacetime de- scribed by the overcharged SV metric includes all the range of the radial coordinate0<R< ∞and is bounded by a singular timelike surface atR = 0.

Charged cosmological black holes: a thorough study of a family of solutions The spacetime de- scribed by the overcharged SV metric includes all the range of the radial coordinate0<R< ∞and is bounded by a singular timelike surface atR = 0

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This paper cites In this case, theAHscorrespondtorootsofthetwosecond-order polynomials, HR 2 +R−m = 0, HR 2−R +m = 0, (49) which can be easily computed.

Charged cosmological black holes: a thorough study of a family of solutions In this case, theAHscorrespondtorootsofthetwosecond-order polynomials, HR 2 +R−m = 0, HR 2−R +m = 0, (49) which can be easily computed

Reference 9

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This paper cites It is bounded from below by the lineσ2 = 1, from above by the curve forσ2 c+, and from the right by the curve for σ2 c−.

Charged cosmological black holes: a thorough study of a family of solutions It is bounded from below by the lineσ2 = 1, from above by the curve forσ2 c+, and from the right by the curve for σ2 c−

Reference 10

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This paper cites An analysis of the roots of Eq.

Charged cosmological black holes: a thorough study of a family of solutions An analysis of the roots of Eq

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This paper cites Analogously, if there existsδ >0 such that Fδ +(ti,t ) = ∫ t ti e(B+δ)u∆H(u) du, (71) converges ast→∞ , then a black-hole/white-hole pair is present.

Charged cosmological black holes: a thorough study of a family of solutions Analogously, if there existsδ >0 such that Fδ +(ti,t ) = ∫ t ti e(B+δ)u∆H(u) du, (71) converges ast→∞ , then a black-hole/white-hole pair is present

Reference 13

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This paper cites In spacetimes represented by Region II there is no AH, and the patch covered by the coordinates is anti-trapped everywhere, therefore there is no doubt about the causal structure.

Charged cosmological black holes: a thorough study of a family of solutions In spacetimes represented by Region II there is no AH, and the patch covered by the coordinates is anti-trapped everywhere, therefore there is no doubt about the causal structure

Reference 15

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This paper cites Following the reasoning of Sec.

Charged cosmological black holes: a thorough study of a family of solutions Following the reasoning of Sec

Reference 16

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This paper cites 2, represents an undercharged case with q < mand small mH0.

Charged cosmological black holes: a thorough study of a family of solutions 2, represents an undercharged case with q < mand small mH0

Reference 17

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This paper cites The singularity at R = m +√ m2−q2 is still present, however no AH is formed and the singularity is naked, as can be seen in Fig.

Charged cosmological black holes: a thorough study of a family of solutions The singularity at R = m +√ m2−q2 is still present, however no AH is formed and the singularity is naked, as can be seen in Fig

Reference 18

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This paper cites They present three AHs, a singularity at 14 R = 0 and an initial singularity att = 0, as shown in Fig.

Charged cosmological black holes: a thorough study of a family of solutions They present three AHs, a singularity at 14 R = 0 and an initial singularity att = 0, as shown in Fig

Reference 19

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This paper cites The Cauchy surface is not present either, as it can be seen in Fig.

Charged cosmological black holes: a thorough study of a family of solutions The Cauchy surface is not present either, as it can be seen in Fig

Reference 20

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This paper cites This case correspondstotheverticalaxisinFig.1, andtheSVmet- ric (37) asymptotes to the Reissner–Nordström metric at large times.

Charged cosmological black holes: a thorough study of a family of solutions This case correspondstotheverticalaxisinFig.1, andtheSVmet- ric (37) asymptotes to the Reissner–Nordström metric at large times

Reference 22

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This paper cites The ﬁrst case, for values ofm2 > q2, presents two apparent horizons R+ and R− and an initial singular- ity atS+.

Charged cosmological black holes: a thorough study of a family of solutions The ﬁrst case, for values ofm2 > q2, presents two apparent horizons R+ and R− and an initial singular- ity atS+

Reference 23

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Charged cosmological black holes: a thorough study of a family of solutions GW151226: Observation of Gravitational Waves from a 22-Solar-Mass Binary Black Hole Coalescence

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Charged cosmological black holes: a thorough study of a family of solutions Akiyamaet al

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Charged cosmological black holes: a thorough study of a family of solutions Superradiance -- the 2020 Edition

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Charged cosmological black holes: a thorough study of a family of solutions Evolving black hole horizons in General Relativity and alternative gravity

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Charged cosmological black holes: a thorough study of a family of solutions Trapped surfaces

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Charged cosmological black holes: a thorough study of a family of solutions On the generalization of McVittie's model for an inhomogeneity in a cosmological spacetime

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Charged cosmological black holes: a thorough study of a family of solutions McVittie's Legacy: Black Holes in an Expanding Universe

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Charged cosmological black holes: a thorough study of a family of solutions More on McVittie's Legacy: A Schwarzschild - de Sitter black and white hole embedded in an asymptotically $\Lambda$CDM cosmology

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Charged cosmological black holes: a thorough study of a family of solutions How the expansion of the universe determines the causal structure of McVittie spacetimes

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Charged cosmological black holes: a thorough study of a family of solutions The McVittie solution with a negative cosmological constant

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Charged cosmological black holes: a thorough study of a family of solutions Making sense of the bizarre behaviour of horizons in the McVittie spacetime

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Charged cosmological black holes: a thorough study of a family of solutions 19,191(1968)

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Charged cosmological black holes: a thorough study of a family of solutions Kastor and J

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Charged cosmological black holes: a thorough study of a family of solutions Nakao, T

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Charged cosmological black holes: a thorough study of a family of solutions Chimento and D

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Charged cosmological black holes: a thorough study of a family of solutions Static Charged Black Hole Solutions in Horava-Lifshitz Gravity

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Charged cosmological black holes: a thorough study of a family of solutions The charged McVittie spacetime

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Charged cosmological black holes: a thorough study of a family of solutions Charged black holes in expanding Einstein-de Sitter universes

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Charged cosmological black holes: a thorough study of a family of solutions Cosmological Solutions with Charged Black Holes

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Charged cosmological black holes: a thorough study of a family of solutions Cuscuton: A Causal Field Theory with an Infinite Speed of Sound

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Observation 7fa81f86-38d2-46b1-a76d-c5ebcf5cf803 · outbound

This paper cites Reissner-Nordstr\"om Metric in the Friedman-Robertson-Walker Universe.

Charged cosmological black holes: a thorough study of a family of solutions Reissner-Nordstr\"om Metric in the Friedman-Robertson-Walker Universe

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-14T13:38:02.094732Z

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Observation 16a389a1-c4c0-49e3-92f4-19a0bd369790 · outbound

This paper cites Cosmological black holes from self-gravitating fields.

Charged cosmological black holes: a thorough study of a family of solutions Cosmological black holes from self-gravitating fields

Reference 52

Resolution: verified exact; local_arxiv, observed 2026-08-14T13:38:02.418128Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 93e6edc7-f8a8-41c1-95d9-3ce09e8d2dc5 · outbound

This paper cites Hamiltonian analysis of the cuscuton.

Charged cosmological black holes: a thorough study of a family of solutions Hamiltonian analysis of the cuscuton

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-14T13:38:02.104560Z

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Observation 84bdab68-0781-4c69-b6d2-3e215ca6e7f2 · outbound

This paper cites an unresolved cited work.

Charged cosmological black holes: a thorough study of a family of solutions Unresolved cited work

Reference 54

Resolution: unresolved; raw_fallback, observed 2026-08-14T13:38:03.196593Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 833937ad-fd99-46cc-ba27-6ee6e5d257c0 · outbound

This paper cites Carrera and D.

Charged cosmological black holes: a thorough study of a family of solutions Carrera and D

Reference 55

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:38:03.180715Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation d9d470e5-f7e1-49f2-a1b7-17b034a1794c · outbound

This paper cites Is the Hawking quasilocal energy "Newtonian"?.

Charged cosmological black holes: a thorough study of a family of solutions Is the Hawking quasilocal energy "Newtonian"?

Reference 56

Resolution: metadata mismatch; local_arxiv, observed 2026-08-14T13:38:02.379088Z

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No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation b4797a19-d30e-4991-862c-436767ffbd61 · outbound

This paper cites Self-gravitating fluid solutions of Shape Dynamics.

Charged cosmological black holes: a thorough study of a family of solutions Self-gravitating fluid solutions of Shape Dynamics

Reference 57

Resolution: verified exact; local_arxiv, observed 2026-08-14T13:38:02.355770Z

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No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 3de5d13a-4d60-4403-a0b3-6764da4a76df · outbound

This paper cites Spherically symmetric spacetimes with a trapped surface.

Charged cosmological black holes: a thorough study of a family of solutions Spherically symmetric spacetimes with a trapped surface

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-14T13:38:02.128332Z

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Observation f8195184-3185-4392-8654-7124efe4f215 · outbound

This paper cites Schnetter and B.

Charged cosmological black holes: a thorough study of a family of solutions Schnetter and B

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-14T13:38:02.133489Z

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Unavailable: canonical work link unavailable.

Observation 792c0525-c69e-4a82-9d2d-0955165fdb4a · outbound

This paper cites A dual null formalism for the collapse of fluids in a cosmological background.

Charged cosmological black holes: a thorough study of a family of solutions A dual null formalism for the collapse of fluids in a cosmological background

Reference 60

Resolution: verified exact; local_arxiv, observed 2026-08-14T13:38:02.317023Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation ae73261b-0299-40c8-9cf1-bedade057ff3 · outbound

This paper cites Quasilocal approach to general universal horizons.

Charged cosmological black holes: a thorough study of a family of solutions Quasilocal approach to general universal horizons

Reference 61

Resolution: verified exact; local_arxiv, observed 2026-08-14T13:38:02.294042Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 17b32d22-4716-4ff9-b91b-e958381a11ef · outbound

This paper cites Quasilocal energy in modified gravity.

Charged cosmological black holes: a thorough study of a family of solutions Quasilocal energy in modified gravity

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-14T13:38:02.148251Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b87ea5da-2ac7-45a5-be3b-60b8cd656d41 · outbound

This paper cites Revisiting the Birkhoff theorem from a dual null point of view.

Charged cosmological black holes: a thorough study of a family of solutions Revisiting the Birkhoff theorem from a dual null point of view

Reference 63

Resolution: verified exact; local_arxiv, observed 2026-08-14T13:38:02.253954Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 98426cd6-3b38-4a8c-b1b5-1f8d4d1494b0 · outbound

This paper cites Cosmological black holes and white holes with time-dependent mass.

Charged cosmological black holes: a thorough study of a family of solutions Cosmological black holes and white holes with time-dependent mass

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-14T13:38:02.158500Z

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Observation 94fdf1ec-3375-4537-bbe4-128baa23bf2d · outbound

This paper cites Walker, J.

Charged cosmological black holes: a thorough study of a family of solutions Walker, J

Reference 65

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:38:03.154449Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 8cb37c5b-3886-4128-8f48-9f531b0486fc · outbound

This paper cites Laue and M.

Charged cosmological black holes: a thorough study of a family of solutions Laue and M

Reference 66

Resolution: verified fuzzy; raw_fallback, observed 2026-08-14T13:38:03.138525Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation a3cb4d22-bb59-4ef0-a09a-a84b35e27576 · outbound

This paper cites Local existence of dynamical and trapping horizons.

Charged cosmological black holes: a thorough study of a family of solutions Local existence of dynamical and trapping horizons

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-14T13:38:02.173264Z

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