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Big Bang Nucleosynthesis with $f(R)$ gravity scalarons and astrophysical consequences

Cosmology and Nongalactic Astrophysics · Submitted 18 Apr 2024

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

The authors' main claim It is found that for a range of scalaron mass $(2.2-3.5) \times 10^4$ eV, the abundance of lithium is lowered by $3-4$ times the value predicted by general relativistic BBN which is a level desired to address the cosmological lithium problem.

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arXiv ID2404.12084 (version 2)
Pith IDPX47WTC7, Pith's permanent record of this paper and its review
CitationAbhijit Talukdar, Sanjeev Kalita. "Big Bang Nucleosynthesis with $f(R)$ gravity scalarons and astrophysical consequences." arXiv:2404.12084 (2024). https://pith.science/paper/PX47WTC7
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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-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 7,673 input tokens.

What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.87 · human participants 0.01 · controlled comparison 0.60 · randomized assignment 0.01 · states quantitative result 0.99 · compares with prior results 0.92 · mentions code or data availability 0.03.

The abstract, sentence by sentence

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

$f(R)$ gravity is one of the serious alternatives of general relativity having a large range of astronomical consequences. In this work, we study Big Bang Nucleosynthesis (BBN) in $f(R)$ gravity theory. We consider modification to gravity due to the existence of primordial black holes in the radiation era which introduce additional degrees of freedom known as scalarons. We calculate the light element abundances by using the BBN code PArthENoPE. It is found that for a range of scalaron mass $(2.2-3.5) \times 10^4$ eV, the abundance of lithium is lowered by $3-4$ times the value predicted by general relativistic BBN which is a level desired to address the cosmological lithium problem. For the above scalaron mass range the helium abundance is within the observed bound. However, the deuterium abundance is found to be increased by $3-6$ times the observed primordial abundance. It calls for a high efficiency of stellar formation and evolution processes for destruction of primordial deuterium which is suggested as possible in scalaron gravity. A novel relation between scalaron mass and black hole mass has been used to show that the above scalaron mass range corresponds to primordial black holes of sub-planetary mass ($\sim 10^{19}$ g) serving as one of the potential candidates of non-baryonic dark matter. We infer Big Bang equivalence of power law $f(R)$ gravity with primordial black holes that are detectable with upcoming gravitational wave detectors.

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 $f(R)$ gravity is one of the serious alternatives of general relativity having a large range of astronomical consequences. background 1.00 0.04 0.02 asserted 0.99
s1 In this work, we study Big Bang Nucleosynthesis (BBN) in $f(R)$ gravity theory. contribution 1.00 0.87 0.02 asserted 0.77
s2 We consider modification to gravity due to the existence of primordial black holes in the radiation era which introduce additional degrees of freedom known as scalarons. contribution 0.70 0.29 0.03 asserted 0.96
s3 We calculate the light element abundances by using the BBN code PArthENoPE. method 1.00 0.93 0.02 asserted 0.99
s4 It is found that for a range of scalaron mass $(2.2-3.5) \times 10^4$ eV, the abundance of lithium is lowered by $3-4$ times the value predicted by general relativistic BBN which is a level desired to address the cosmological lithium problem. result 0.99 0.94 0.53 asserted 1.00
s5 For the above scalaron mass range the helium abundance is within the observed bound. result 1.00 0.91 0.07 asserted 0.99
s6 However, the deuterium abundance is found to be increased by $3-6$ times the observed primordial abundance. result 0.97 0.96 0.13 asserted 1.00
s7 It calls for a high efficiency of stellar formation and evolution processes for destruction of primordial deuterium which is suggested as possible in scalaron gravity. interpretation 0.95 0.25 0.09 hedged possibility 0.99
s8 A novel relation between scalaron mass and black hole mass has been used to show that the above scalaron mass range corresponds to primordial black holes of sub-planetary mass ($\sim 10^{19}$ g) serving as one of the potential candidates of non-baryonic dark matter. interpretation 0.53 0.82 0.24 asserted 0.68
s9 We infer Big Bang equivalence of power law $f(R)$ gravity with primordial black holes that are detectable with upcoming gravitational wave detectors. interpretation 0.68 0.79 0.28 asserted 0.72

What kind of paper the classifier reports this is: simulation study 0.62 · evidence from simulation or computation 1.00.

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sources read
  • arXiv listing abstract v2
not examined
  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers
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  • 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

$f(R)$ gravity is one of the serious alternatives of general relativity having a large range of astronomical consequences. In this work, we study Big Bang Nucleosynthesis (BBN) in $f(R)$ gravity theory. We consider modification to gravity due to the existence of primordial black holes in the radiation era which introduce additional degrees of freedom known as scalarons. We calculate the light element abundances by using the BBN code PArthENoPE. It is found that for a range of scalaron mass $(2.2-3.5) \times 10^4$ eV, the abundance of lithium is lowered by $3-4$ times the value predicted by general relativistic BBN which is a level desired to address the cosmological lithium problem. For the above scalaron mass range the helium abundance is within the observed bound. However, the deuterium abundance is found to be increased by $3-6$ times the observed primordial abundance. It calls for a high efficiency of stellar formation and evolution processes for destruction of primordial deuterium which is suggested as possible in scalaron gravity. A novel relation between scalaron mass and black hole mass has been used to show that the above scalaron mass range corresponds to primordial black holes of sub-planetary mass ($\sim 10^{19}$ g) serving as one of the potential candidates of non-baryonic dark matter. We infer Big Bang equivalence of power law $f(R)$ gravity with primordial black holes that are detectable with upcoming gravitational wave detectors.

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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

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Cites as support 1 paper
Cites as background 1 paper
  • Distinguishing between these two is one of the major goals of ongoing Dark Energy Survey [ref] and the upcoming Euclid mission [ref] .

    Euclid Definition Study Report · Introduction · 0.97

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