Asosiy kontentga oʻtish
AkademScholar
Muassasalar

Indian Institute of Science Education and Research, Tirupati

Nom variantlari: IISER · IISER Tirupati

Davlat:
IN
ROR:
https://ror.org/032d0e990
3
h-indeks
30
Iqtiboslar
22
Asarlar
11
Mualliflar
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Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
035810035810201820202021202220232024202520262018: Nashrlar 1, Iqtiboslar 02020: Nashrlar 1, Iqtiboslar 02021: Nashrlar 3, Iqtiboslar 02022: Nashrlar 6, Iqtiboslar 52023: Nashrlar 2, Iqtiboslar 82024: Nashrlar 6, Iqtiboslar 92025: Nashrlar 2, Iqtiboslar 12026: Nashrlar 1, Iqtiboslar 7

Iqtibos tarixi

035810201820202021202220232024202520262018: Iqtiboslar 02020: Iqtiboslar 02021: Iqtiboslar 02022: Iqtiboslar 52023: Iqtiboslar 82024: Iqtiboslar 92025: Iqtiboslar 12026: Iqtiboslar 7

Nashr tarixi

035810201820202021202220232024202520262018: Nashrlar 12020: Nashrlar 12021: Nashrlar 32022: Nashrlar 62023: Nashrlar 22024: Nashrlar 62025: Nashrlar 22026: Nashrlar 1

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

01345201820202021202220232024202520262018: h-indeks 02020: h-indeks 02021: h-indeks 02022: h-indeks 12023: h-indeks 22024: h-indeks 22025: h-indeks 32026: h-indeks 3

Eng koʻp iqtibos qilingan asarlar

  1. Nonlinear Reconstruction of Images from Patterns Generated by Deterministic or Random Optical Masks—Concepts and Review of Research20223 iqtibos
  2. Non-Linear Reconstruction of Images from Patterns Generated by Deterministic or Random Optical Masks – Concepts and Review of Research20222 iqtibos
  3. Observation of Strong Nuclear Suppression in Exclusive <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>J</mml:mi><mml:mo>/</mml:mo><mml:mi>ψ</mml:mi></mml:mrow></mml:math> Photoproduction in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>Au</mml:mi><mml:mo stretchy="false">+</mml:mo><mml:mi>Au</mml:mi></mml:mrow></mml:math> Ultraperipheral Collisions at RHIC20242 iqtibos
  4. Exclusive <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>J</mml:mi><mml:mo>/</mml:mo><mml:mi>ψ</mml:mi></mml:mrow><mml:mo>,</mml:mo><mml:mo> </mml:mo><mml:mrow><mml:mi>ψ</mml:mi><mml:mo>(</mml:mo><mml:mn>2</mml:mn><mml:mi>s</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math>, and <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:msup><mml:mi>e</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:msup><mml:mi>e</mml:mi><mml:mo>−</mml:mo></mml:msup></mml:mrow></mml:math> pair production in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>Au</mml:mi><mml:mo>+</mml:mo><mml:mi>Au</mml:mi></mml:mrow></mml:math> ultraperipheral collisions at the BNL Relativistic Heavy Ion Collider20242 iqtibos
  5. Evidence of Mass Ordering of Charm and Bottom Quark Energy Loss in Au+Au Collisions at RHIC20220 iqtibos
  6. Light nuclei collectivity from s NN = 3 GeV Au+Au collisions at RHIC20220 iqtibos
  7. Erratum to: Evidence of Mass Ordering of Charm and Bottom Quark Energy Loss in Au+Au Collisions at RHIC20230 iqtibos
  8. Production of protons and light nuclei in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mi>Au</mml:mi><mml:mo>+</mml:mo><mml:mi>Au</mml:mi></mml:math> collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:msqrt><mml:msub><mml:mi>s</mml:mi><mml:mrow><mml:mi>N</mml:mi><mml:mi>N</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mspace width="0.16em"/><mml:mo>=</mml:mo><mml:mspace width="0.16em"/><mml:mn>3</mml:mn></mml:mrow></mml:math> GeV with the STAR detector20240 iqtibos
  9. Strangeness production in $$ \sqrt{s_{\textrm{NN}}} $$ = 3 GeV Au+Au collisions at RHIC20240 iqtibos
  10. Correlations of event activity with hard and soft processes in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:mi>p</mml:mi><mml:mo>+</mml:mo><mml:mtext>Au</mml:mtext></mml:mrow></mml:math> collisions at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"><mml:mrow><mml:msqrt><mml:msub><mml:mi>s</mml:mi><mml:mrow><mml:mi>N</mml:mi><mml:mi>N</mml:mi></mml:mrow></mml:msub></mml:msqrt><mml:mo>=</mml:mo><mml:mn>200</mml:mn></mml:mrow></mml:math> GeV at the RHIC STAR experiment20240 iqtibos