1997
DOI: 10.1016/s0370-2693(97)00152-4
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Search for stable heavy charged particles in e+e− collisions at , 161 and 172 GeV

Abstract: A search for stable or long-lived heavy charged particles in e + e interactions at energies of 130-136, 161 and 172 GeV has been performed using the data taken by the DELPHI experiment at LEP. The search is based on particle identi cation provided by the Time Projection Chamber and the Ring Imaging Cherenkov detector. Upper limits at 95% con dence level are derived on the cross-section for heavy long-lived pair-produced charge e and 2=3e particles in the range of 0.4-2.3 pb for masses from 45 to 84 GeV/c 2 . W… Show more

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Cited by 19 publications
(3 citation statements)
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“…Various searches have been performed to search for such particles [194]. At LEP, limits were set on CLLPs with charges 2 3 Q e , 4 3 Q e , and 5 3 Q e at a range of collision energies from 91 GeV to 209 GeV [162,195,196,197]. At the Tevatron, the CDF experiment set limits on CLLPs with charges 2 3 Q e and 1 3 Q e , excluding masses up to 250 GeV [169].…”
Section: Particles With Anomalous Electric Chargementioning
confidence: 99%
“…Various searches have been performed to search for such particles [194]. At LEP, limits were set on CLLPs with charges 2 3 Q e , 4 3 Q e , and 5 3 Q e at a range of collision energies from 91 GeV to 209 GeV [162,195,196,197]. At the Tevatron, the CDF experiment set limits on CLLPs with charges 2 3 Q e and 1 3 Q e , excluding masses up to 250 GeV [169].…”
Section: Particles With Anomalous Electric Chargementioning
confidence: 99%
“…These are limits are weaker because the coupling of FCPs with Z-boson is suppressed by a sin 2 (θ W ) factor. A search for FCPs with = 2/3 was performed by OPAL using 1991-93 data [17,75,76], which rules out ≥2/3 for mass M < 84GeV .…”
Section: F11 Accelerator Based Experimentsmentioning
confidence: 99%
“…Although the masses of these particles can lie above the reach of current accelerators, experimental constraints on masses and charges of mCPs have been derived from fixed target accelerators [13][14][15][16][17][18][19][20], colliders [21][22][23][24][25][26][27][28], stellar models [3,[29][30][31], cosmic microwave background [29,30,[32][33][34][35][36][37], big-bang nucleosynthesis [30], Supernova 1987A [30,38], neutron stars [39,40], pulsars and gamma ray bursts [41], galaxy clusters [42], the Lamb shift [29,43,44], dark cosmic ray searches [45], positronium decay [46], reactor neutrinos [47,48], and the µ magnetic moment [29]. An early levitation experiment [49] found an indication for the existence for fractional charges that was not confirmed by following efforts [50,…”
mentioning
confidence: 99%