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A. Dauletov

Сўнгги маълум муассаса:
Karakalpak State University
4
h-индекс
1
i10-индекси
39
Иқтибослар
9
Асарлар
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Иқтибос шарҳи

Йиллар бўйича нашрлар (устун) ва иқтибослар (чизиқ)

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03581005101520202520262025: Нашрлар 9, Иқтибослар 192026: Нашрлар 0, Иқтибослар 20

Иқтибос тарихи

05101520202520262025: Иқтибослар 192026: Иқтибослар 20

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035810202520262025: Нашрлар 92026: Нашрлар 0

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01345202520262025: h-индекс 22026: h-индекс 4

Энг кўп иқтибос қилинган асарлар

  1. Black holes in general relativity coupled with nonlinear electrodynamics surrounded by perfect fluid dark matter: Thermodynamics, particle motion, and black hole shadow202518 иқтибос
  2. Possible wormholes in generalized geometry–matter coupling gravity induced by the Dekel–Zhao dark matter profile20255 иқтибос
  3. Traversable Wormholes in f(R) Gravity: Influence of Global Monopole Charge and Energy Conditions20255 иқтибос
  4. Einasto-inspired non-commutative black holes within dark matter galactic halos in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si8.svg" display="inline" id="d1e849"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi mathvariant="double-struck">Q</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> gravity20254 иқтибос
  5. Implication of f(Q,T) gravity on the formation of the charge compact stars and constraining their mass-radius relations in lower mass gap region20254 иқтибос
  6. Thermodynamic constraints and observational validation of the deceleration parameter20251 иқтибос
  7. Role of three coupling parameters on maximum mass and stability: Theoretical insights into relativistic massive compact objects in mass gap under <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si334.svg" display="inline" id="d1e10703"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>Q</mml:mi><mml:mo>,</mml:mo><mml:mi>T</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> action20251 иқтибос
  8. Probing dark energy and cosmic acceleration with f(Q,T) gravity theories20251 иқтибос
  9. Modeling of Finch-Skea hybrid neutron stars with complexity-free characteristics20250 иқтибос