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Mualliflar

N. Herrmann

Soʻnggi maʼlum muassasa:
Heidelberg University
ORCID:
0000-0003-0970-2968
6
h-indeks
4
i10-indeksi
103
Iqtiboslar
20
Asarlar
Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
0134503581020162017201820192021202220232024202520262016: Nashrlar 0, Iqtiboslar 12017: Nashrlar 0, Iqtiboslar 22018: Nashrlar 2, Iqtiboslar 32019: Nashrlar 0, Iqtiboslar 22021: Nashrlar 0, Iqtiboslar 42022: Nashrlar 1, Iqtiboslar 02023: Nashrlar 2, Iqtiboslar 12024: Nashrlar 5, Iqtiboslar 62025: Nashrlar 1, Iqtiboslar 52026: Nashrlar 0, Iqtiboslar 3

Iqtibos tarixi

03581020162017201820192021202220232024202520262016: Iqtiboslar 12017: Iqtiboslar 22018: Iqtiboslar 32019: Iqtiboslar 22021: Iqtiboslar 42022: Iqtiboslar 02023: Iqtiboslar 12024: Iqtiboslar 62025: Iqtiboslar 52026: Iqtiboslar 3

Nashr tarixi

0134520162017201820192021202220232024202520262016: Nashrlar 02017: Nashrlar 02018: Nashrlar 22019: Nashrlar 02021: Nashrlar 02022: Nashrlar 12023: Nashrlar 22024: Nashrlar 52025: Nashrlar 12026: Nashrlar 0

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

03581020162017201820192021202220232024202520262016: h-indeks 62017: h-indeks 62018: h-indeks 62019: h-indeks 62021: h-indeks 62022: h-indeks 62023: h-indeks 62024: h-indeks 62025: h-indeks 62026: 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. Beam energy dependence of rapidity-even dipolar flow in Au+Au collisions20180 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
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