Noncommutative Schwarzschild black hole surrounded by quintessence: Thermodynamics, Shadows and Quasinormal modes

B. C. L\"utf\"uo\u{g}lu; B. Hamil

RECORD

Noncommutative Schwarzschild black hole surrounded by quintessence: Thermodynamics, Shadows and Quasinormal modes

B. Hamil, B. C. Lütfüoğlu

General Relativity and Quantum Cosmology · Submitted 17 Jan 2024

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

The authors' main claim After visualizing these results qualitatively, we calculated the quasinormal modes in WKB and Mashhoon approximations and we demonstrated the impacts of quintessence matter and noncommutative spacetime on the whole quantities.

how it is stated · asserted 1.00 read the record →

Comment (0) Read on arXiv ↗

Cite ▾

arXiv ID2401.09295 (version 3)

Pith IDIGRLYZYG, Pith's permanent record of this paper and its review

CitationB. C. L\"utf\"uo\u{g}lu, B. Hamil. "Noncommutative Schwarzschild black hole surrounded by quintessence: Thermodynamics, Shadows and Quasinormal modes." arXiv:2401.09295 (2024). https://pith.science/paper/IGRLYZYG

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-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 5,624 input tokens.

What the abstract itself states, as probabilities: claims first 0.05 · states limitation 0.07 · human participants 0.01 · controlled comparison 0.15 · randomized assignment 0.01 · states quantitative result 0.06 · compares with prior results 0.61 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v3. Results and the main claim are underlined; show every role.

{In (Sci. Rep. \textbf{12}, 8516 (2022)), Campos et al studied} the quasinormal modes and shadows of noncommutative Schwarzschild black holes. Since we know that the quintessence matter surrounding black holes has { significant effects} on the black hole quantities, {in this study, we aimed to show this influence by revisiting the same problem in the presence of quintessence matter field. To this end, we first examined the thermodynamics of noncommutative Schwarzschild black holes embedded in quintessence matter using Hawking temperature, entropy, and specific heat functions. After that,} we discussed phase transition and stability { features. We then investigated} the shadow images in the presence of plasma. After visualizing these results qualitatively, we calculated the quasinormal modes in WKB and Mashhoon approximations and we demonstrated the impacts of quintessence matter and noncommutative spacetime on the whole quantities.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#	sentence	role	the authors' own work	states the main conclusion	strength
s0	{In (Sci. Rep.	background 1.00	0.03	0.01	unclear 0.98
s1	\textbf{12}, 8516 (2022)), Campos et al studied} the quasinormal modes and shadows of noncommutative Schwarzschild black holes.	background 1.00	0.03	0.03	asserted 0.99
s2	Since we know that the quintessence matter surrounding black holes has { significant effects} on the black hole quantities, {in this study, we aimed to show this influence by revisiting the same problem in the presence of quintessence matter field.	contribution 0.80	0.33	0.10	asserted 0.99
s3	To this end, we first examined the thermodynamics of noncommutative Schwarzschild black holes embedded in quintessence matter using Hawking temperature, entropy, and specific heat functions.	method 0.71	0.95	0.05	asserted 0.94
s4	After that,} we discussed phase transition and stability { features.	contribution 0.73	0.91	0.04	asserted 0.62
s5	We then investigated} the shadow images in the presence of plasma.	contribution 0.78	0.93	0.04	asserted 0.95
s6	After visualizing these results qualitatively, we calculated the quasinormal modes in WKB and Mashhoon approximations and we demonstrated the impacts of quintessence matter and noncommutative spacetime on the whole quantities.	contribution 0.45	0.96	0.56	asserted 1.00

What kind of paper the classifier reports this is: theoretical result 0.88 · evidence from proof or derivation 0.55.

What was examined, and what was not

sources read

arXiv listing abstract v3

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

{In (Sci. Rep. \textbf{12}, 8516 (2022)), Campos et al studied} the quasinormal modes and shadows of noncommutative Schwarzschild black holes. Since we know that the quintessence matter surrounding black holes has { significant effects} on the black hole quantities, {in this study, we aimed to show this influence by revisiting the same problem in the presence of quintessence matter field. To this end, we first examined the thermodynamics of noncommutative Schwarzschild black holes embedded in quintessence matter using Hawking temperature, entropy, and specific heat functions. After that,} we discussed phase transition and stability { features. We then investigated} the shadow images in the presence of plasma. After visualizing these results qualitatively, we calculated the quasinormal modes in WKB and Mashhoon approximations and we demonstrated the impacts of quintessence matter and noncommutative spacetime on the whole quantities.

Human review

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

References

How the literature uses it

10 arXiv papers cite this in 10 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 · 4 sentences without a confident label

Uses its method or tool 1 paper

As mentioned above, the effective potential exhibits well-behaved characteristics, which justifies the use of the WKB semi-classical approximation to compute the corresponding quasi-normal mode (QNM) frequencies (see Refs. [ref] and references therein).

Black hole physics within $f(R)$ gravity: Quasi-normal spectra and greybody factors · The WKB approximation · 0.85

Cites it as background 5 papers

As a result, a substantial number of studies have focused on the QNMs for various models of quantum-corrected black holes [ref] .

Long-lived Quasinormal modes around regular black holes and wormholes in Covariant Effective Quantum Gravity · Introduction · 0.91
Recently various Kiselev BHs have been proposed and widely studied [ref]

Kiselev Black holes in quantum fluctuation modified gravity · Introduction · 0.88
Different aspects of BH thermodynamics in Moyal spacetime have been extensively investigated using these deformed BH solutions [ref] .

Thermodynamics and phase transitions of $\kappa$-deformed Schwarzschild-AdS black holes · Introduction · 0.95

What it cites

Cites as background 6 papers

Recently, in [ref] authors examined the QNMs of the Schwarzschild-like black holes.

Quasinormal Modes in Noncommutative Schwarzschild black holes · Introduction · 0.96
In general, the QNMs can be derived within two methodologies: perturbing the metric [ref] , or coupling fields to the spacetime and considering the interactions between the black hole and the fields [ref] .

Gravitational probe of quantum spacetime · Quasinormal modes · 0.90
In general, the QNMs can be derived within two methodologies: perturbing the metric [ref] , or coupling fields to the spacetime and considering the interactions between the black hole and the fields [ref] .

Metric perturbations in Noncommutative Gravity · Quasinormal modes · 0.90

Discussion

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