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Search for Production of Invisible Final States in Single-Photon Decays of Upsilon(1S)

P. del Amo Sanchez

TL;DR

No evidence for processes in the mass range m(A⁰) ≤ 9.2 GeV and m(χ) ≤ 4.5 GeV is found in the sample of 98 × 10⁶ Υ(2S) decays collected with the BABAR detector and stringent limits on new physics models that contain light dark matter states are set.

Abstract

We search for single-photon decays of the Upsilon(1S) resonance, Upsilon->gamma+invisible, where the invisible state is either a particle of definite mass, such as a light Higgs boson A0, or a pair of dark matter particles, chi chi-bar. Both A0 and chi are assumed to have zero spin. We tag Upsilon(1S) decays with a dipion transition Upsilon(2S)->pi+pi-Upsilon(1S) and look for events with a single energetic photon and significant missing energy. We find no evidence for such processes in the mass range m_A0<=9.2 GeV and m_chi<=4.5 GeV in the sample of 98e6 Upsilon(2S) decays collected with the BaBar detector and set stringent limits on new physics models that contain light dark matter states.

Search for Production of Invisible Final States in Single-Photon Decays of Upsilon(1S)

TL;DR

No evidence for processes in the mass range m(A⁰) ≤ 9.2 GeV and m(χ) ≤ 4.5 GeV is found in the sample of 98 × 10⁶ Υ(2S) decays collected with the BABAR detector and stringent limits on new physics models that contain light dark matter states are set.

Abstract

We search for single-photon decays of the Upsilon(1S) resonance, Upsilon->gamma+invisible, where the invisible state is either a particle of definite mass, such as a light Higgs boson A0, or a pair of dark matter particles, chi chi-bar. Both A0 and chi are assumed to have zero spin. We tag Upsilon(1S) decays with a dipion transition Upsilon(2S)->pi+pi-Upsilon(1S) and look for events with a single energetic photon and significant missing energy. We find no evidence for such processes in the mass range m_A0<=9.2 GeV and m_chi<=4.5 GeV in the sample of 98e6 Upsilon(2S) decays collected with the BaBar detector and set stringent limits on new physics models that contain light dark matter states.

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