Asosiy kontentga oʻtish
AkademScholar

Mahsulotlar

Ishlab chiquvchilar uchun

AkademBasetez oradaDasturchilar API
Mualliflar

M. Csanád

Ism variantlari: Máté Csanád

Soʻnggi maʼlum muassasa:
Eötvös Loránd University
ORCID:
0000-0002-3154-6925
6
h-indeks
2
i10-indeksi
122
Iqtiboslar
37
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
013450613192520152017201920202021202220232024202520262015: Nashrlar 0, Iqtiboslar 112017: Nashrlar 2, Iqtiboslar 02019: Nashrlar 1, Iqtiboslar 12020: Nashrlar 1, Iqtiboslar 62021: Nashrlar 2, Iqtiboslar 152022: Nashrlar 3, Iqtiboslar 202023: Nashrlar 2, Iqtiboslar 212024: Nashrlar 5, Iqtiboslar 182025: Nashrlar 1, Iqtiboslar 22026: Nashrlar 0, Iqtiboslar 8

Iqtibos tarixi

0613192520152017201920202021202220232024202520262015: Iqtiboslar 112017: Iqtiboslar 02019: Iqtiboslar 12020: Iqtiboslar 62021: Iqtiboslar 152022: Iqtiboslar 202023: Iqtiboslar 212024: Iqtiboslar 182025: Iqtiboslar 22026: Iqtiboslar 8

Nashr tarixi

0134520152017201920202021202220232024202520262015: Nashrlar 02017: Nashrlar 22019: Nashrlar 12020: Nashrlar 12021: Nashrlar 22022: Nashrlar 32023: Nashrlar 22024: Nashrlar 52025: Nashrlar 12026: Nashrlar 0

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020152017201920202021202220232024202520262015: h-indeks 22017: h-indeks 22019: h-indeks 22020: h-indeks 32021: h-indeks 32022: h-indeks 42023: h-indeks 52024: h-indeks 52025: h-indeks 52026: h-indeks 6

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. Elastic Scattering and Total Cross-Section in p+p Reactions20120 iqtibos
  4. Evidence of Mass Ordering of Charm and Bottom Quark Energy Loss in Au+Au Collisions at RHIC20220 iqtibos
  5. Erratum to: Evidence of Mass Ordering of Charm and Bottom Quark Energy Loss in Au+Au Collisions at RHIC20230 iqtibos
  6. 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
  7. Strangeness production in $$ \sqrt{s_{\textrm{NN}}} $$ = 3 GeV Au+Au collisions at RHIC20240 iqtibos
  8. 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
  9. 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
AkademIndex'da koʻrish →