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Jurnal

Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields

ISSN:
0556-2821
2
h-indeks
14
Iqtiboslar
10
Asarlar

Ishonch signallari

1 dan 3 signal mavjud

Mustaqil ijobiy signallar — yagona “predator/qonuniy” hukmi emas, balki yaqinlashuvchi tasvir.

  • DOAJ
    Maʼlumot yoʻq
    doaj.org
  • OAK roʻyxati
    Maʼlumot yoʻq
    OAK
  • Yaroqli ISSN
    Mavjud
    ISSN

Bu axborot yorligʻi, rasmiy qaror emas. Signal yoʻqligi jazo emas — masalan, mintaqaviy jurnal DOAJ'da boʻlmasligi mumkin.

Vaqt boʻyicha

Vaqt boʻyicha tahlil

Iqtibos sharhi

Yillar boʻyicha nashrlar (ustun) va iqtiboslar (chiziq)

  • Nashrlar
  • Iqtiboslar
013450119982001200220062007200920132014201820231998: Nashrlar 3, Iqtiboslar 02001: Nashrlar 0, Iqtiboslar 12002: Nashrlar 1, Iqtiboslar 02006: Nashrlar 0, Iqtiboslar 12007: Nashrlar 0, Iqtiboslar 12009: Nashrlar 0, Iqtiboslar 12013: Nashrlar 0, Iqtiboslar 12014: Nashrlar 0, Iqtiboslar 12018: Nashrlar 0, Iqtiboslar 12023: Nashrlar 0, Iqtiboslar 1

Iqtibos tarixi

0119982001200220062007200920132014201820231998: Iqtiboslar 02001: Iqtiboslar 12002: Iqtiboslar 02006: Iqtiboslar 12007: Iqtiboslar 12009: Iqtiboslar 12013: Iqtiboslar 12014: Iqtiboslar 12018: Iqtiboslar 12023: Iqtiboslar 1

Nashr tarixi

0134519982001200220062007200920132014201820231998: Nashrlar 32001: Nashrlar 02002: Nashrlar 12006: Nashrlar 02007: Nashrlar 02009: Nashrlar 02013: Nashrlar 02014: Nashrlar 02018: Nashrlar 02023: Nashrlar 0

h-indeks evolyutsiyasi

Yillar boʻyicha jamlangan h-indeks

01219982001200220062007200920132014201820231998: h-indeks 12001: h-indeks 12002: h-indeks 12006: h-indeks 12007: h-indeks 12009: h-indeks 12013: h-indeks 22014: h-indeks 22018: h-indeks 22023: h-indeks 2

Eng koʻp iqtibos qilingan asarlar

  1. Charged-particle multiplicity and angular distributions in proton-emulsion interactions at 800 GeV19874 iqtibos
  2. Multiplicity of secondary particles in inelastic proton-neon interactions at 300 GeV/<i>c</i>19814 iqtibos
  3. Direct measurement of the top quark mass by the DØ Collaboration19982 iqtibos
  4. Study of correlations between secondary protons produced in proton-neon interactions at 300 GeV/<i>c</i>19841 iqtibos
  5. Neutral-strange-particle production in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>p</mml:mi><mml:mi/><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">Ne</mml:mi></mml:mrow><mml:mprescripts/><mml:mrow/><mml:mrow><mml:mn>20</mml:mn></mml:mrow><mml:mrow/><mml:mrow/></mml:mmultiscripts></mml:mrow></mml:math>and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>pN</mml:mi></mml:math>interactions at 300 GeV19911 iqtibos
  6. Cumulative particle production in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>p</mml:mi><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi mathvariant="normal">Ne</mml:mi></mml:mrow><mml:mprescripts/><mml:mrow/><mml:mrow><mml:mn>20</mml:mn></mml:mrow><mml:mrow/><mml:mrow/></mml:mmultiscripts></mml:mrow></mml:math>interactions at 300 GeV19921 iqtibos
  7. On the<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mrow><mml:mover><mml:mrow><mml:mi>τ</mml:mi></mml:mrow><mml:mrow><mml:mo>→</mml:mo></mml:mrow></mml:mover></mml:mrow></mml:mrow><mml:mi>VP</mml:mi><mml:mrow><mml:msub><mml:mrow><mml:mi>ν</mml:mi></mml:mrow><mml:mrow><mml:mi>τ</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math>decays19981 iqtibos
  8. Right-handed currents and strong interactions at short distances19780 iqtibos
  9. Limits on anomalous<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>WW</mml:mi><mml:mi>γ</mml:mi></mml:math>and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>WWZ</mml:mi></mml:math>couplings19980 iqtibos
  10. Double logarithms,<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msup><mml:mrow><mml:mi mathvariant="normal">ln</mml:mi></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:msup></mml:mrow><mml:mn/><mml:mo>(</mml:mo><mml:mn>1</mml:mn><mml:mo>/</mml:mo><mml:mi>x</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:math>and the NLO Dokshitzer-Gribov-Lipatov-Altarelli-Parisi evolution for the nonsinglet component of the nucleon spin structure function<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi>g</mml:mi></mml:mrow><mml:mrow><mml:mn>1</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math>20020 iqtibos
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