Asosiy kontentga oʻtish
AkademScholar
Mualliflar

Orhan Dönmez

Soʻnggi maʼlum muassasa:
American University of the Middle East
ORCID:
0000-0001-9017-2452
12
h-indeks
15
i10-indeksi
386
Iqtiboslar
73
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
01325385005010015020020042006201220132014202120222024202520262004: Nashrlar 1, Iqtiboslar 02006: Nashrlar 1, Iqtiboslar 02012: Nashrlar 1, Iqtiboslar 02013: Nashrlar 1, Iqtiboslar 02014: Nashrlar 1, Iqtiboslar 02021: Nashrlar 1, Iqtiboslar 12022: Nashrlar 2, Iqtiboslar 12024: Nashrlar 21, Iqtiboslar 212025: Nashrlar 18, Iqtiboslar 1632026: Nashrlar 26, Iqtiboslar 200

Iqtibos tarixi

05010015020020042006201220132014202120222024202520262004: Iqtiboslar 02006: Iqtiboslar 02012: Iqtiboslar 02013: Iqtiboslar 02014: Iqtiboslar 02021: Iqtiboslar 12022: Iqtiboslar 12024: Iqtiboslar 212025: Iqtiboslar 1632026: Iqtiboslar 200

Nashr tarixi

01325385020042006201220132014202120222024202520262004: Nashrlar 12006: Nashrlar 12012: Nashrlar 12013: Nashrlar 12014: Nashrlar 12021: Nashrlar 12022: Nashrlar 22024: Nashrlar 212025: Nashrlar 182026: Nashrlar 26

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0510152020042006201220132014202120222024202520262004: h-indeks 02006: h-indeks 02012: h-indeks 02013: h-indeks 02014: h-indeks 02021: h-indeks 12022: h-indeks 12024: h-indeks 32025: h-indeks 82026: h-indeks 12

Eng koʻp iqtibos qilingan asarlar

  1. Linear redshift parametrization of deceleration parameter in f(R,Lm) gravity202414 iqtibos
  2. Constraining <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si140.svg" display="inline" id="d1e319"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi>Q</mml:mi> <mml:mo>,</mml:mo> <mml:msub> <mml:mrow> <mml:mi>L</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>m</mml:mi> </mml:mrow> </mml:msub> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> gravity with bulk viscosity202514 iqtibos
  3. Exploring accelerated expansion in the universe: A study of <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si274.svg" display="inline" id="d1e325"><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> gravity with parameterized EoS and cosmological constraints202413 iqtibos
  4. Observational constraints on the equation of state of viscous fluid in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si250.svg" display="inline" id="d1e314"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>,</mml:mo><mml:mi>T</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> gravity202410 iqtibos
  5. Testing quantum-corrected black holes with QPOs observations: a study of particle dynamics and accretion flow202510 iqtibos
  6. Late-time cosmology in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si23.svg" display="inline" id="d1e469"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>Q</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mrow><mml:mi>L</mml:mi></mml:mrow><mml:mrow><mml:mi>m</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math> gravity: Analytical solutions and observational fits20249 iqtibos
  7. Model-independent parameterization of H(z) and its implications for cosmic evolution20249 iqtibos
  8. Possible wormholes in generalized geometry–matter coupling gravity induced by the Dekel–Zhao dark matter profile20258 iqtibos
  9. Dehnen-type dark matter wormholes in the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" altimg="si1.svg" display="inline" id="d1e414"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mrow> <mml:mo>(</mml:mo> <mml:mi mathvariant="script">R</mml:mi> <mml:mo>,</mml:mo> <mml:msub> <mml:mrow> <mml:mi mathvariant="script">L</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>m</mml:mi> </mml:mrow> </mml:msub> <mml:mo>,</mml:mo> <mml:mi mathvariant="script">T</mml:mi> <mml:mo>)</mml:mo> </mml:mrow> </mml:mrow> </mml:math> action20258 iqtibos
  10. Testing strong gravitational field using the Johannsen–Psaltis metric: Bondi–Hoyle–Lyttleton accretion model and QPO studies20267 iqtibos

Hammualliflar

  1. Farruh Atamurotov16 ta umumiy asar2025–2026
  2. Javlon Rayimbaev15 ta umumiy asar2024–2026
  3. G. Mustafa13 ta umumiy asarSkelet yozuvlar: 12024–2026
  4. M. Koussour13 ta umumiy asarSkelet yozuvlar: 12024–2025
  5. S. Muminov13 ta umumiy asar2024–2026
  6. Abdelmalek Bouzenada11 ta umumiy asar2025–2026
  7. Abdelghani Errehymy9 ta umumiy asarSkelet yozuvlar: 52024–2026
  8. S. K. Maurya8 ta umumiy asarSkelet yozuvlar: 22024–2026
  9. Yerlan Myrzakulov7 ta umumiy asar2024–2026
  10. M. Yousaf7 ta umumiy asar2025–2026

Barcha hammualliflar →