Interacting HDE and NADE in Brans-Dicke Chameleon Cosmology

Ahmad Sheykhi; Mubasher Jamil

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Interacting HDE and NADE in Brans-Dicke Chameleon Cosmology

Ahmad Sheykhi, Mubasher Jamil

High Energy Physics - Theory · Submitted 3 Oct 2010

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

The authors' main claim We find out that in this model the phantom crossing can be constructed if the model parameters are chosen suitably.

how it is stated · asserted 0.76 read the record →

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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.

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Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 3,646 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.05 · states limitation 0.09 · human participants 0.01 · controlled comparison 0.03 · randomized assignment 0.01 · states quantitative result 0.05 · compares with prior results 0.21 · mentions code or data availability 0.01.

The abstract, sentence by sentence

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

Motivated by the recent work of one of us [1], we generalize this work to the case where the pressureless dark matter and the holographic dark energy do not conserve separately but interact with each other. We investigate the cosmological applications of interacting holographic dark energy in Brans-Dicke theory with chameleon scalar field which is non-minimally coupled to the matter field. We find out that in this model the phantom crossing can be constructed if the model parameters are chosen suitably. We also perform the study for the new agegraphic dark energy model and calculate some relevant cosmological parameters and their evolution.

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	Motivated by the recent work of one of us [1], we generalize this work to the case where the pressureless dark matter and the holographic dark energy do not conserve separately but interact with each other.	contribution 0.74	0.54	0.05	asserted 0.87
s1	We investigate the cosmological applications of interacting holographic dark energy in Brans-Dicke theory with chameleon scalar field which is non-minimally coupled to the matter field.	contribution 0.98	0.66	0.06	asserted 0.87
s2	We find out that in this model the phantom crossing can be constructed if the model parameters are chosen suitably.	result 1.00	0.96	0.55	asserted 0.76
s3	We also perform the study for the new agegraphic dark energy model and calculate some relevant cosmological parameters and their evolution.	contribution 0.98	0.95	0.07	asserted 0.99

What kind of paper the classifier reports this is: theoretical result 0.99 · evidence from proof or derivation 0.83.

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

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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

Motivated by the recent work of one of us [1], we generalize this work to the case where the pressureless dark matter and the holographic dark energy do not conserve separately but interact with each other. We investigate the cosmological applications of interacting holographic dark energy in Brans-Dicke theory with chameleon scalar field which is non-minimally coupled to the matter field. We find out that in this model the phantom crossing can be constructed if the model parameters are chosen suitably. We also perform the study for the new agegraphic dark energy model and calculate some relevant cosmological parameters and their evolution.

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4 arXiv papers cite this in 4 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

Cites it as background 4 papers

Reconstructing the holographic and agegraphic scalar field models of DE is one of interesting issue which has been investigated in the literature [ref] .

Reconstructing interacting entropy-corrected holographic scalar field models of dark energy in non-flat universe · Introduction · 0.93
Quintessence [ref] , phantom (ghost) field [ref] , K-essence [ref] , Chaplygin gas [ref] , holographic dark energy which originates from quantum gravity [ref] and agegraphic DE [ref] are some examples of DE models with time varying EoS parameter.

Ghost dark energy with sign-changeable interaction term · Introduction · 0.95
Although the nature of both $DM$ and $DE$ still remains a mystery, the possibility that DE and DM can interact with each other has been widely discussed recently [ref] .

(m,n)-type holographic dark energy models · holographic dark energy with interaction · 1.00

What it cites · 5 sentences without a confident label

Cites as background 1 paper

Other studies on the chameleon gravity have been carried out in [ref] .

Chameleon Dark Energy · Introduction · 1.00

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