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On the search for artificial Dyson-like structures around pulsars

Popular Physics · Submitted 18 May 2015

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

The authors' main claim This indicates that the search for infrared ring-like sources close to slowly rotating pulsars seems to be quite promising.

how it is stated · hedged possibility 0.99 read the record →

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arXiv ID1505.05131 (version 3)
Pith ID2DD37XMB, Pith's permanent record of this paper and its review
CitationZ. Osmanov. "On the search for artificial Dyson-like structures around pulsars." arXiv:1505.05131 (2015). https://pith.science/paper/2DD37XMB
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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, 5,625 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.92 · human participants 0.01 · controlled comparison 0.04 · randomized assignment 0.01 · states quantitative result 0.98 · compares with prior results 0.29 · mentions code or data availability 0.01.

The abstract, sentence by sentence

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

Assuming the possibility of existence of a supercivilization we extend the idea of Freeman Dyson considering pulsars instead of stars. It is shown that instead of a spherical shell the supercivilization must use ring-like constructions. We have found that a size of the "ring" should be of the order of $(10^{-4}-10^{-1})$AU with temperature interval $(300-600)$K for relatively slowly rotating pulsars and $(10-350)$AU with temperature interval $(300-700)$K for rapidly spinning neutron stars, respectively. Although for the latter the Dyson construction is unrealistically massive and cannot be considered seriously. Analyzing the stresses in terms of the radiation and wind flows it has been argued that they cannot significantly affect the ring construction. On the other hand, the ring in-plane unstable equilibrium can be restored by the energy which is small compared to the energy extracted from the star. This indicates that the search for infrared ring-like sources close to slowly rotating pulsars seems to be quite promising.

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 Assuming the possibility of existence of a supercivilization we extend the idea of Freeman Dyson considering pulsars instead of stars. background 0.53 0.45 0.04 hedged possibility 0.60
s1 It is shown that instead of a spherical shell the supercivilization must use ring-like constructions. result 0.93 0.74 0.42 asserted 1.00
s2 We have found that a size of the "ring" should be of the order of $(10^{-4}-10^{-1})$AU with temperature interval $(300-600)$K for relatively slowly rotating pulsars and $(10-350)$AU with temperature interval $(300-700)$K for rapidly spinning neutron stars, respectively. result 1.00 0.93 0.24 asserted 1.00
s3 Although for the latter the Dyson construction is unrealistically massive and cannot be considered seriously. limitation 0.63 0.58 0.08 asserted 0.99
s4 Analyzing the stresses in terms of the radiation and wind flows it has been argued that they cannot significantly affect the ring construction. result 0.76 0.68 0.04 asserted 0.76
s5 On the other hand, the ring in-plane unstable equilibrium can be restored by the energy which is small compared to the energy extracted from the star. result 0.66 0.68 0.08 asserted 0.65
s6 This indicates that the search for infrared ring-like sources close to slowly rotating pulsars seems to be quite promising. interpretation 0.74 0.51 0.84 hedged possibility 0.99

What kind of paper the classifier reports this is: theoretical result 0.99 · evidence from proof or derivation 0.52.

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

Assuming the possibility of existence of a supercivilization we extend the idea of Freeman Dyson considering pulsars instead of stars. It is shown that instead of a spherical shell the supercivilization must use ring-like constructions. We have found that a size of the "ring" should be of the order of $(10^{-4}-10^{-1})$AU with temperature interval $(300-600)$K for relatively slowly rotating pulsars and $(10-350)$AU with temperature interval $(300-700)$K for rapidly spinning neutron stars, respectively. Although for the latter the Dyson construction is unrealistically massive and cannot be considered seriously. Analyzing the stresses in terms of the radiation and wind flows it has been argued that they cannot significantly affect the ring construction. On the other hand, the ring in-plane unstable equilibrium can be restored by the energy which is small compared to the energy extracted from the star. This indicates that the search for infrared ring-like sources close to slowly rotating pulsars seems to be quite promising.

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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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