1991
DOI: 10.1070/pu1991v034n05abeh002492
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Interaction of the electron and the positron in pair production

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Cited by 103 publications
(101 citation statements)
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“…Long time ago it has been pointed out that final state Coulomb corrections to the Born cross section have to be taken into account in the case of pointlike charged fermion pair production [8]. This Coulomb correction has been usually introduced as an enhancement factor, C in Eq.…”
Section: σ(E + E − → Bb) At Thresholdmentioning
confidence: 99%
“…Long time ago it has been pointed out that final state Coulomb corrections to the Born cross section have to be taken into account in the case of pointlike charged fermion pair production [8]. This Coulomb correction has been usually introduced as an enhancement factor, C in Eq.…”
Section: σ(E + E − → Bb) At Thresholdmentioning
confidence: 99%
“…If new particles possess new y-charge, interacting with massless bosons or intermediate bosons with sufficiently small mass (y-interaction), for slow y-charged particles a Coulomb-like factor of "Gamov-Sommerfeld-Sakharov enhancement" [65][66][67] should be added in the annihilation cross section…”
Section: Self-interacting Dark Mattermentioning
confidence: 99%
“…[231] in the framework of perturbation theory. Note that here R denotes the distance between OHe and the nucleus and not radius of the nucleus, as it was in Equations (65), (66), (68), and (69).…”
Section: Ohe Atoms and Their Interaction With Nucleimentioning
confidence: 99%
“…If new particles possess new y-charge, interacting with massless bosons or intermediate bosons with sufficiently small mass (y-interaction), for slow y-charged particles Coulomb-like factor of "Gamov-Sommerfeld-Sakharov enhancement" [36][37][38] should be added in the annihilation cross section…”
Section: 27mentioning
confidence: 99%