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Search for chargino and neutralino production at \(\sqrt{s} = 189\) GeV at LEP

  • Experimental physics
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Abstract.

A search for charginos and neutralinos, predicted by supersymmetric theories, is performed using a data sample of 182.1 pb\(^{-1}\) taken at a centre-of-mass energy of 189 GeV with the OPAL detector at LEP. No evidence for chargino or neutralino production is found. Upper limits on chargino and neutralino pair production (\(\tilde{\chi}^+_1 \tilde{\chi}^-_1\), \(\tilde{\chi}^0 _1 \tilde{\chi}^0 _2\)) cross-sections are obtained as a function of the chargino mass (\(m_{\tilde{\chi}^\pm_1}\)), the lightest neutralino mass (\(m_{\tilde{\chi}^0 _1}\)) and the second lightest neutralino mass (\(m_{\tilde{\chi}^0 _2}\)). Within the Constrained Minimal Supersymmetric Standard Model framework, and for \(m_{\tilde{\chi}^\pm_1} - m_{\tilde{\chi}^0 _1} \geq 5\) GeV, the 95% confidence level lower limits on \(m_{\tilde{\chi}^\pm_1}\) are 93.6 GeV for \(\tan \beta = 1.5\) and 94.1 GeV for \(\tan \beta = 35\). These limits are obtained assuming a universal scalar mass \(m_0 \geq\) 500 GeV. The corresponding limits for all \(m_0\) are 78.0 and 71.7 GeV. The 95% confidence level lower limits on the lightest neutralino mass, valid for any value of \(\tan \beta\) are 32.8 GeV for \(m_0 \geq 500\) GeV and 31.6 GeV for all \(m_0\).

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Received: 14 October 1999 / Published online: 6 March 2000

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The OPAL Collaboration., Abbiendi et al., G. Search for chargino and neutralino production at \(\sqrt{s} = 189\) GeV at LEP. Eur. Phys. J. C 14, 187–198 (2000). https://doi.org/10.1007/s100520000346

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  • DOI: https://doi.org/10.1007/s100520000346

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