Asosiy kontentga oʻtish
AkademScholar
Muassasalar

Indian Institute of Technology Patna

Nom variantlari: IIT Patna · IITP

Davlat:
IN
ROR:
https://ror.org/01ft5vz71
3
h-indeks
60
Iqtiboslar
32
Asarlar
45
Mualliflar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0358100613192520172018201920202021202220232024202520262017: Nashrlar 2, Iqtiboslar 02018: Nashrlar 4, Iqtiboslar 02019: Nashrlar 1, Iqtiboslar 02020: Nashrlar 2, Iqtiboslar 02021: Nashrlar 2, Iqtiboslar 02022: Nashrlar 5, Iqtiboslar 02023: Nashrlar 4, Iqtiboslar 72024: Nashrlar 8, Iqtiboslar 232025: Nashrlar 1, Iqtiboslar 202026: Nashrlar 0, Iqtiboslar 10

Iqtibos tarixi

0613192520172018201920202021202220232024202520262017: Iqtiboslar 02018: Iqtiboslar 02019: Iqtiboslar 02020: Iqtiboslar 02021: Iqtiboslar 02022: Iqtiboslar 02023: Iqtiboslar 72024: Iqtiboslar 232025: Iqtiboslar 202026: Iqtiboslar 10

Nashr tarixi

03581020172018201920202021202220232024202520262017: Nashrlar 22018: Nashrlar 42019: Nashrlar 12020: Nashrlar 22021: Nashrlar 22022: Nashrlar 52023: Nashrlar 42024: Nashrlar 82025: Nashrlar 12026: Nashrlar 0

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

0134520172018201920202021202220232024202520262017: h-indeks 02018: h-indeks 02019: h-indeks 02020: h-indeks 02021: h-indeks 02022: h-indeks 02023: 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. 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
  4. Strangeness production in $$ \sqrt{s_{\textrm{NN}}} $$ = 3 GeV Au+Au collisions at RHIC20240 iqtibos
  5. 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
  6. Results on elastic cross sections in proton–proton collisions at s=510 GeV with the STAR detector at RHIC20240 iqtibos