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AkademScholar

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Identifikatsiya

Ishlab chiquvchilar uchun

Ekotizim

Muassasalar

Indian Institute of Science Education and Research, Bhopal

Nom variantlari: IISER · IISER - Bhopal · IISER-B

Davlat:
IN
ROR:
https://ror.org/02rb21j89
3
h-indeks
24
Iqtiboslar
15
Asarlar
17
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0134503581020162017201820192021202220232024202520262016: Nashrlar 0, Iqtiboslar 12017: Nashrlar 0, Iqtiboslar 12018: Nashrlar 2, Iqtiboslar 02019: Nashrlar 1, Iqtiboslar 02021: Nashrlar 2, Iqtiboslar 02022: Nashrlar 0, Iqtiboslar 42023: Nashrlar 0, Iqtiboslar 52024: Nashrlar 5, Iqtiboslar 52025: Nashrlar 2, Iqtiboslar 22026: Nashrlar 1, Iqtiboslar 6

Iqtibos tarixi

03581020162017201820192021202220232024202520262016: Iqtiboslar 12017: Iqtiboslar 12018: Iqtiboslar 02019: Iqtiboslar 02021: Iqtiboslar 02022: Iqtiboslar 42023: Iqtiboslar 52024: Iqtiboslar 52025: Iqtiboslar 22026: Iqtiboslar 6

Nashr tarixi

0134520162017201820192021202220232024202520262016: Nashrlar 02017: Nashrlar 02018: Nashrlar 22019: Nashrlar 12021: Nashrlar 22022: Nashrlar 02023: Nashrlar 02024: Nashrlar 52025: Nashrlar 22026: Nashrlar 1

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520162017201820192021202220232024202520262016: h-indeks 12017: h-indeks 12018: h-indeks 12019: h-indeks 12021: h-indeks 12022: h-indeks 22023: h-indeks 22024: h-indeks 22025: h-indeks 32026: h-indeks 3

Eng koʻp iqtibos qilingan asarlar

  1. 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
  2. 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
  3. Classifying meteorites with <scp>MetNet</scp> : A deep learning approach using reflectance spectroscopy20251 iqtibos
  4. 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
  5. Strangeness production in $$ \sqrt{s_{\textrm{NN}}} $$ = 3 GeV Au+Au collisions at RHIC20240 iqtibos
  6. 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
  7. Measurement of directed flow 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> 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>19.6</mml:mn></mml:mrow></mml:math> and 27 GeV with the STAR event plane detector20250 iqtibos
  8. Dynamical response of twin stars to perturbations20260 iqtibos