kth.sePublications KTH
Change search
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • ieee
  • modern-language-association-8th-edition
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf
Observation of 𝑡⁢¯𝑡 Production in Pb+Pb Collisions at √𝑠NN=5.02  TeV with the ATLAS Detector
CPPM, Aix-Marseille Université, CNRS/IN2P3, Marseille, France.ORCID iD: 0000-0002-6665-4934
KTH, School of Engineering Sciences (SCI), Physics, Particle Physics, Astrophysics and Medical Imaging.ORCID iD: 0000-0002-9605-3558
KTH, School of Engineering Sciences (SCI), Physics, Particle Physics, Astrophysics and Medical Imaging.ORCID iD: 0000-0001-9415-7903
KTH, School of Engineering Sciences (SCI), Physics, Particle Physics, Astrophysics and Medical Imaging.ORCID iD: 0009-0004-1439-5151
Show others and affiliations
Number of Authors: 28402025 (English)In: Physical Review Letters, ISSN 0031-9007, E-ISSN 1079-7114, Vol. 134, no 14, article id 142301Article in journal (Refereed) Published
Abstract [en]

Top-quark pair production is observed in lead-lead (Pb + Pb) collisions at root s(NN) = 5.02 TeV at the Large Hadron Collider with the ATLAS detector. The data sample was recorded in 2015 and 2018, amounting to an integrated luminosity of 1.9 nb(-1). Events with exactly one electron and one muon and at least two jets are selected. Top-quark pair production is measured with an observed (expected) significance of 5.0 (4.1) standard deviations. The measured top-quark pair production cross section is sigma(t (t) over bar) = 3.6(-0.09)(+1.0) (stat)(-0.5)(+0.8) (syst) mu b, with a total relative uncertainty of 31%, and is consistent with theoretical predictions using a range of different nuclear parton distribution functions. The observation of this process consolidates the evidence of the existence of all quark flavors in the preequilibrium stage of the quark-gluon plasma at very high energy densities, similar to the conditions present in the early Universe.

Place, publisher, year, edition, pages
American Physical Society (APS) , 2025. Vol. 134, no 14, article id 142301
National Category
Subatomic Physics
Identifiers
URN: urn:nbn:se:kth:diva-373570DOI: 10.1103/PhysRevLett.134.142301ISI: 001498373100001PubMedID: 40279599Scopus ID: 2-s2.0-105003765541OAI: oai:DiVA.org:kth-373570DiVA, id: diva2:2018307
Note

QC 20251202

Available from: 2025-12-02 Created: 2025-12-02 Last updated: 2025-12-02Bibliographically approved

Open Access in DiVA

No full text in DiVA

Other links

Publisher's full textPubMedScopus

Authority records

Dimitriadi, ChristinaLeopold, AlexanderLundberg, OlofLund-Jensen, BengtOhm, Christian C.Shaheen, RabiaStrandberg, JonasVande Voorde, U. Magdalena

Search in DiVA

By author/editor
Aad, G.Dimitriadi, ChristinaLeopold, AlexanderLundberg, OlofLund-Jensen, BengtOhm, Christian C.Shaheen, RabiaStrandberg, JonasVande Voorde, U. MagdalenaZwalinski, L.
By organisation
Particle Physics, Astrophysics and Medical Imaging
In the same journal
Physical Review Letters
Subatomic Physics

Search outside of DiVA

GoogleGoogle Scholar

doi
pubmed
urn-nbn

Altmetric score

doi
pubmed
urn-nbn
Total: 16 hits
CiteExportLink to record
Permanent link

Direct link
Cite
Citation style
  • apa
  • ieee
  • modern-language-association-8th-edition
  • vancouver
  • Other style
More styles
Language
  • de-DE
  • en-GB
  • en-US
  • fi-FI
  • nn-NO
  • nn-NB
  • sv-SE
  • Other locale
More languages
Output format
  • html
  • text
  • asciidoc
  • rtf