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024 7 _ |a 10.1007/s100520050392
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024 7 _ |a 1434-6044
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024 7 _ |a 1434-6052
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024 7 _ |a 10.1007/PL00021667
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037 _ _ |a PUBDB-2017-09808
041 _ _ |a English
082 _ _ |a 530
088 1 _ |a DESY-98-077; YUMS-98-10; SNUTP-98-52; PM-98-14; IFT-9-98; YUMS-98--10; SNUTP-98--52; DESY-98--77; PM-98--14; hep-ph/9806279
088 _ _ |a DESY-98-077
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088 _ _ |a hep-ph/9806279
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100 1 _ |a Choi, S. Y.
|0 P:(DE-HGF)0
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245 _ _ |a Chargino pair production in $e^+ e^-$ collisions
260 _ _ |a Berlin
|c 1999
|b Springer
336 7 _ |a article
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336 7 _ |a Journal Article
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500 _ _ |a F-Bereich; Theorie
520 _ _ |a Charginos $\chi_1^\pm$ are expected to be the lightest observable supersymmetric particles in many supersymmetric models. We present a procedure which will allow to determine the chargino mixing angles and, subsequently, the fundamental SUSY parameters $M_2, \mu$ and $\tan\beta$ by measurements of the total cross section and the spin correlations in $e^+e^-$ annihilation to $\chi_1^+ \chi_1^-$ chargino pairs.
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650 _ 7 |a electron positron: annihilation
|2 INSPIRE
650 _ 7 |a supersymmetry
|2 INSPIRE
650 _ 7 |a sparticle: pair production
|2 INSPIRE
650 _ 7 |a chargino: polarization
|2 INSPIRE
650 _ 7 |a chargino: mixing angle
|2 INSPIRE
650 _ 7 |a spin: correlation
|2 INSPIRE
650 _ 7 |a chargino: decay
|2 INSPIRE
650 _ 7 |a angular correlation
|2 INSPIRE
650 _ 7 |a spin: density matrix
|2 INSPIRE
650 _ 7 |a CP: violation
|2 INSPIRE
650 _ 7 |a channel cross section: energy dependence
|2 INSPIRE
650 _ 7 |a angular distribution
|2 INSPIRE
650 _ 7 |a polarization: angular dependence
|2 INSPIRE
650 _ 7 |a polarization: longitudinal
|2 INSPIRE
650 _ 7 |a polarization: transverse
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650 _ 7 |a numerical calculations
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693 _ _ |0 EXP:(DE-MLZ)NOSPEC-20140101
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700 1 _ |a Djouadi, A.
|0 P:(DE-HGF)0
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700 1 _ |a Dreiner, Herbert K.
|0 P:(DE-HGF)0
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700 1 _ |a Kalinowski, J.
|0 P:(DE-HGF)0
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700 1 _ |a Zerwas, Peter
|0 P:(DE-H253)PIP1001086
|b 4
773 _ _ |a 10.1007/PL00021667
|g Vol. 7, no. 1, p. 123 -
|0 PERI:(DE-600)1459069-4
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|p 123 - 134
|t The @European physical journal / C
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