Quark Production Cross Section $-$ Accelerator Searches

INSPIRE   PDGID:
S027C
X-SECT (cm${}^{2}$) CHG ${\mathrm {(\mathit e/3)}}$ MASS ${\mathrm {(GeV)}}$ ENERGY ${\mathrm {(GeV)}}$ BEAM EVTS DOCUMENT ID TECN
$ \text{<1.7-2.3E-39} $ $\pm2$ $100 - 600$ $7000$ ${{\mathit p}}{{\mathit p}}$ 0 1
CHATRCHYAN
2013AR
CMS
$ \text{<14-5.4E-39} $ $\pm1$ $100 - 600$ $7000$ ${{\mathit p}}{{\mathit p}}$ 0 1
CHATRCHYAN
2013AR
CMS
$ \text{<1.3E-36} $ $\pm2$ $45 - 84$ $130 - 172$ ${{\mathit e}^{+}}{{\mathit e}^{-}}$ 0
ABREU
1997D
DLPH
$ \text{<2.E-35} $ $+2$ $250$ $1800$ ${{\mathit p}}{{\overline{\mathit p}}}$ 0 2
ABE
1992J
CDF
$ \text{<1.E-35} $ $+4$ $250$ $1800$ ${{\mathit p}}{{\overline{\mathit p}}}$ 0 2
ABE
1992J
CDF
$ \text{<3.8E-28} $ 14.5A ${}^{28}\mathrm {Si}-$Pb 0 3
HE
1991
PLAS
$ \text{<3.2E-28} $ 14.5A ${}^{28}\mathrm {Si}-$Cu 0 3
HE
1991
PLAS
$ \text{<1.E-40} $ $\pm1$,2 <10 ${{\mathit p}},{{\mathit \nu}},{{\overline{\mathit \nu}}}$ 0
BERGSMA
1984B
CHRM
$ \text{<1.E-36} $ $\pm1$,2 <9 $200$ ${{\mathit \mu}}$ 0
AUBERT
1983C
SPEC
$ \text{<2.E-10} $ $\pm2$,4 1$-$3 $200$ ${{\mathit p}}$ 0 4
BUSSIERE
1980
CNTR
$ \text{<5.E-38} $ $+1$,2 >5 $300$ ${{\mathit p}}$ 0 5, 6
STEVENSON
1979
CNTR
$ \text{<1.E-33} $ $\pm1$ <20 $52$ ${{\mathit p}}{{\mathit p}}$ 0
BASILE
1978
SPEC
$ \text{<9.E-39} $ $\pm1$,2 <6 $400$ ${{\mathit p}}$ 0 5
ANTREASYAN
1977
SPEC
$ \text{<8.E-35} $ $+1$,2 <20 $52$ ${{\mathit p}}{{\mathit p}}$ 0 7
FABJAN
1975
CNTR
$ \text{<5.E-38} $ $-1$,2 4$-$9 $200$ ${{\mathit p}}$ 0
NASH
1974
CNTR
$ \text{<1.E-32} $ $+2$,4 4$-$24 $52$ ${{\mathit p}}{{\mathit p}}$ 0
ALPER
1973
SPEC
$ \text{<5.E-31} $ $+1$,2,4 <12 $300$ ${{\mathit p}}$ 0
LEIPUNER
1973
CNTR
$ \text{<6.E-34} $ $\pm1$,2 <13 $52$ ${{\mathit p}}{{\mathit p}}$ 0
BOTT
1972
CNTR
$ \text{<1.E-36} $ $-4$ $4$ $70$ ${{\mathit p}}$ 0
ANTIPOV
1971
CNTR
$ \text{<1.E-35} $ $\pm1$,2 $2$ $28$ ${{\mathit p}}$ 0 8
ALLABY
1969B
CNTR
$ \text{<4.E-37} $ $-2$ <5 $70$ ${{\mathit p}}$ 0 4
ANTIPOV
1969
CNTR
$ \text{<3.E-37} $ $-1$,2 2$-$5 $70$ ${{\mathit p}}$ 0 8
ANTIPOV
1969B
CNTR
$ \text{<1.E-35} $ $+1$,2 <7 $30$ ${{\mathit p}}$ 0
DORFAN
1965
CNTR
$ \text{<2.E-35} $ $-2$ $<2.5-$5 $30$ ${{\mathit p}}$ 0 9
FRANZINI
1965B
CNTR
$ \text{<5.E-35} $ $+1$,2 <2.2 $21$ ${{\mathit p}}$ 0
BINGHAM
1964
HLBC
$ \text{<1.E-32} $ $+1$,2 <4.0 $28$ ${{\mathit p}}$ 0
BLUM
1964
HBC
$ \text{<1.E-35} $ $+1$,2 <2.5 $31$ ${{\mathit p}}$ 0 9
HAGOPIAN
1964
HBC
$ \text{<1.E-34} $ $+1$ <2 $28$ ${{\mathit p}}$ 0
LEIPUNER
1964
CNTR
$ \text{<1.E-33} $ $+1$,2 <2.4 $24$ ${{\mathit p}}$ 0
MORRISON
1964
HBC
1  CHATRCHYAN 2013AR limits assume pair-produced long-lived spin-1/2 particles neutral under SU(3)$_{C}$ and SU(2)$_{L}$.
2  ABE 1992J flux limits decrease as the mass increases from 50 to 500 GeV.
3  HE 1991 limits are for charges of the form $\mathit N\pm1$/3 from 23/3 to 38/3.
4  Hadronic or leptonic quarks.
5  Cross section cm${}^{2}$/GeV${}^{2}$.
6  $3 \times 10^{-5}$ $<$lifetime $<1 \times 10^{-3}$ s.
7  Includes BOTT 1972 results.
8  Assumes isotropic cm production.
9  Cross section inferred from flux.
References