Primordial Black Holes and Cosmological Phase Transitions Report ...

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$Kawasaki dynamic in continuum Math. Encounters XXXV ... - CCM$

PBHs and Cosmological Phase Transitions 44 Table 9: The SMPP particles and their supersymmetric partners (sparticles) according to the MSSM. Note, however, that before EW symmetry breaking the γ (superpartner photino) and Z 0 (superpartner zino) fields are decomposed into a B (superpartner: Bino ˜ B) and W 0 (superpartner: Wino ˜ W 0 ) fields. Particle Symbol Spin Sparticle Symbol Spin electron e 1/2 selectron ˜e 0 muon µ 1/2 smuon ˜µ 0 tau τ 1/2 stau ˜τ 0 electron neutrino νe 1/2 selectron sneutrino ˜νe 0 muon neutrino νµ 1/2 smuon sneutrino νµ ˜ 0 tau neutrino top ντ t 1/2 1/2 stau sneutrino stop ντ ˜ ˜t 0 0 bottom b 1/2 sbottom ˜b 0 charm c 1/2 scharm ˜c 0 strange s 1/2 sstrange ˜s 0 up u 1/2 sup ũ 0 down d 1/2 sdown d˜ 0 photon γ 1 photino ˜γ 1/2 W W ± 1 Wino ˜ W 0 1/2 Z Z 0 1 Zino ˜ Z 1/2 gluon g 1 gluino ˜g 1/2 Higgs H 0 Higgsino ˜ H 1/2
PBHs and Cosmological Phase Transitions 45 eigenstates with charge ±1 called charginos. We will denote the neutralino and chargino mass eigenstates by Ñi (i =1, 2, 3, 4) and ˜ C ± i (i =1, 2) 19 . By convention, these are labeled in ascending order, so that mÑ1
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Contents List of Figures vii List o
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Table 49 (continued). PBHs and Cosm
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Table 49 (continued). Radiation EW
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