Pith. Sign in

RECORD

Dilaton Black Holes with Electric Charge

PaperPDF from arXiv

data files

Paper breakdownThe authors' claims, conditions and measurements, as JSON Signed receiptProof this review has not been altered
X Bluesky LinkedIn Reddit Hacker News
Malik Rakhmanov

High Energy Physics - Theory · Submitted 26 Oct 1993

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim It is shown that in most cases the scalar curvature is divergent at the horizons.

how it is stated · asserted 0.99 read the record →

Comment (0) Read on arXiv ↗
Cite ▾
arXiv IDhep-th/9310174 (version 2)
Pith IDYG7PDBJK, Pith's permanent record of this paper and its review
CitationMalik Rakhmanov. "Dilaton Black Holes with Electric Charge." arXiv:hep-th/9310174 (1993). https://pith.science/paper/YG7PDBJK
Claim paper

The compiled record

The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

Open the compiled record

Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,781 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.48 · human participants 0.01 · controlled comparison 0.03 · randomized assignment 0.01 · states quantitative result 0.14 · compares with prior results 0.70 · mentions code or data availability 0.01.

The abstract, sentence by sentence

arXiv listing abstract v2. Results and the main claim are underlined; .

Static spherically symmetric solutions of the Einstein-Maxwell gravity with the dilaton field are described. The solutions correspond to black holes and are generalizations of the previously known dilaton black hole solution. In addition to mass and electric charge these solutions are labeled by a new parameter, the dilaton charge of the black hole. Different effects of the dilaton charge on the geometry of space-time of such black holes are studied. It is shown that in most cases the scalar curvature is divergent at the horizons. Another feature of the dilaton black hole is that there is a finite interval of values of electric charge for which no black hole can exist.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 Static spherically symmetric solutions of the Einstein-Maxwell gravity with the dilaton field are described. contribution 0.94 0.79 0.05 asserted 0.99
s1 The solutions correspond to black holes and are generalizations of the previously known dilaton black hole solution. contribution 0.49 0.63 0.12 asserted 1.00
s2 In addition to mass and electric charge these solutions are labeled by a new parameter, the dilaton charge of the black hole. contribution 0.53 0.82 0.17 asserted 1.00
s3 Different effects of the dilaton charge on the geometry of space-time of such black holes are studied. contribution 0.99 0.90 0.07 asserted 0.55
s4 It is shown that in most cases the scalar curvature is divergent at the horizons. result 1.00 0.93 0.26 asserted 0.99
s5 Another feature of the dilaton black hole is that there is a finite interval of values of electric charge for which no black hole can exist. result 1.00 0.88 0.22 asserted 1.00

What kind of paper the classifier reports this is: theoretical result 1.00 · evidence from proof or derivation 1.00.

What was examined, and what was not

sources read
  • arXiv listing abstract v2
not examined
  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers
levels run
  • P abstract
not run
  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
Original abstract

Static spherically symmetric solutions of the Einstein-Maxwell gravity with the dilaton field are described. The solutions correspond to black holes and are generalizations of the previously known dilaton black hole solution. In addition to mass and electric charge these solutions are labeled by a new parameter, the dilaton charge of the black hole. Different effects of the dilaton charge on the geometry of space-time of such black holes are studied. It is shown that in most cases the scalar curvature is divergent at the horizons. Another feature of the dilaton black hole is that there is a finite interval of values of electric charge for which no black hole can exist.

Human review

How Pith checks papers → · Full audit of this paper →

References
How the literature uses it

6 arXiv papers cite this in 9 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

Papers citing it · 6 sentences without a confident label

Builds on it 1 paper
  • However, in the $(n,p)=(2,0)$ case, even singular geometries that do not satisfy the constraint ([ref]) have some interesting applications [ref] , and our construction generalizes these solutions to all values of $n$ and $p$.

    Multi-charged geometries with cosmological constant · The most general solution for static $p$–branes · 0.97

Cites it as background 2 papers
  • Indeed, besides the well-studied electrically charged black holes in the Einstein-Maxwell theory, the inclusion of scalar fields has been shown to give rise to boson stars [ref] , hairy black holes [ref] , dilaton effects in black holes [ref] , spontaneous scalarization [ref] , and even structural changes in the Cauchy horizon as well as the central singularity of both Kerr and Reissner-Nordström black holes [ref] .[ The scalar-tensor setup of gravity has sparked interest due to the natural emergence of scalar fields in supergravity [ref] and in the low-energy limit of string theory [ref] . ]

    Generating Rotating Spacetime in Ricci-Based Gravity: Naked Singularity as a Black Hole Mimicker · Introduction · 0.94

  • The causal structures and thermodynamic properties of black hole solution with dilaton have been explored in [ref] .

    Test particle motion around black hole in Einstein-Maxwell-scalar theory · Introduction · 1.00

Discussion

Know something about this paper? Leave a comment, or highlight any passage above to comment on it.