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Bayes factor of the ATLAS diphoton excess: using Bayes factors to understand anomalies at the LHC

  • Andrew Fowlie

Research output: Contribution to journalArticleResearchpeer-review

Abstract

As an example of using Bayesian statistics in searches for new physics at the LHC, we present a calculation of Bayes factors for the erstwhile digamma resonance (Ϝ) versus the SM in light of ATLAS 8 TeV 20.3/fb, 13 TeV 3.2/fb and 13 TeV 15.4/fb data. We matched, wherever possible, parameterisations in the ATLAS analysis. We calculated that the plausibility of the Ϝversus the Standard Model increased by about eight in light of the 8 TeV 20.3/fb and 13 TeV 3.2/fb ATLAS data, somewhat justifying interest in Ϝ models. All told, however, in light of 15.4/fb data, the Ϝ was disfavoured by about 0.7. We argue that Bayes factors could play an important role in future anomalies by clarifying the plausibility of new physics and sidestepping look-elsewhere effects.

Original languageEnglish
Article number46
Number of pages7
JournalThe European Physical Journal Plus
Volume132
Issue number1
DOIs
Publication statusPublished - 1 Jan 2017
  • ARC Centre of Excellence for Particle Physics at the Tera-Scale

    Balazs, C. (Primary Chief Investigator (PCI)), Barberio, E. (Chief Investigator (CI)), Bell, N. (Chief Investigator (CI)), Gherghetta, T. (Chief Investigator (CI)), Limosani, A. (Chief Investigator (CI)), Sevior, M. (Chief Investigator (CI)), Taylor, G. (Chief Investigator (CI)), Thomas, A. (Chief Investigator (CI)), Varvell, K. (Chief Investigator (CI)), Volkas, R. R. (Chief Investigator (CI)), Williams, A. G. (Chief Investigator (CI)), Yabsley, B. (Chief Investigator (CI)), Young, R. D. (Chief Investigator (CI)), Clarke, A. (Partner Investigator (PI)), Jakobs, C. (Partner Investigator (PI)), Kruse, M. (Partner Investigator (PI)), Meroni, C. (Partner Investigator (PI)), Parker, M. (Partner Investigator (PI)) & Trodden, M. (Partner Investigator (PI))

    ARC - Australian Research Council

    1/01/1131/12/18

    Project: Research

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