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1990
DOI: 10.1103/physrevlett.65.679
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Millicharged particles

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Cited by 95 publications
(90 citation statements)
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“…Figure 4 shows a graph of charge vs. mass and shaded regions of charge-mass combinations that have been excluded so far by other experiments. 4,7 Shown are regions excluded due to the most precise measurement of the Lamb Shift, and three regions excluded because of particle physics experiments: Mel Schwartz's SLAC Beam Dump experiment, the Fermilab E613 experiment, and the ASP Free Also shown are two regions excluded based on cosmological grounds. Masses below 1 MeV are excluded because of the e ect the existence of mQ particles would have o n n ucleosynthesis: if mQ particles had a very small mass, they would have caused the universe to have cooled more rapidly, and nuclei would have started forming earlier, giving fewer free neutrons the chance to decay, which i n turn would give rise to a higher He abundance than is currently observed.…”
Section: Shadow Universesmentioning
confidence: 99%
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“…Figure 4 shows a graph of charge vs. mass and shaded regions of charge-mass combinations that have been excluded so far by other experiments. 4,7 Shown are regions excluded due to the most precise measurement of the Lamb Shift, and three regions excluded because of particle physics experiments: Mel Schwartz's SLAC Beam Dump experiment, the Fermilab E613 experiment, and the ASP Free Also shown are two regions excluded based on cosmological grounds. Masses below 1 MeV are excluded because of the e ect the existence of mQ particles would have o n n ucleosynthesis: if mQ particles had a very small mass, they would have caused the universe to have cooled more rapidly, and nuclei would have started forming earlier, giving fewer free neutrons the chance to decay, which i n turn would give rise to a higher He abundance than is currently observed.…”
Section: Shadow Universesmentioning
confidence: 99%
“…4,7 They are also not forbidden by established physical principles. In fact, charge quantization is poorly understood, and there is no a-priori reason to assume that all particles need to have a c harge that is an integer multiple of e=3.…”
Section: Why Look For Them?mentioning
confidence: 99%
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“…Although charged dark matter is strongly constrained [1], particles with magnetic and/or electric dipole moments [2], axions [3] and millicharged dark matter [4] are viable dark matter candidates. Another dark matter candidate that can couple to the electromagnetic field is mirror matter.…”
Section: Introductionmentioning
confidence: 99%
“…For one thing, the apparently much stronger astrophysical and cosmological bounds [5][6][7][8][9][10] (for a recent review, see Ref.…”
mentioning
confidence: 99%