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\@writefile{lof}{\contentsline {figure}{\numberline {1}{\ignorespaces {\it  Schematic representation of the SUSY mass spectrum considered in our numerical analysis, where $m_{\mathaccent "707E\relax q}$ and $m_{\mathaccent "707E\relax t}$ denote the masses of the first two and third generations of squarks, respectively. The hierarchy factor $\rho $, the phase $\phi _{\mathaccent "707E\relax {g}}$ of the gluino mass, and the phases $\phi _{A_{t,b}}$ of the soft SUSY breaking trilinear couplings, with $\phi _{A_t} = \phi _{A_b} = \phi _{A_U}$, are varied independently (see also discussion in the text).}}}{30}}
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\@writefile{lof}{\contentsline {figure}{\numberline {4}{\ignorespaces {\it  SM and SUSY Higgs-DP contributions to $\Delta M_{B_d}$ and $\Delta M_{B_s}$ as functions of the gluino phase ${\rm  arg}\, (m_{\mathaccent "707E\relax {g}})$, for $M_{\rm  SUSY} = 1$\nobreakspace  {}TeV, $M_{H^+} = 0.2$\nobreakspace  {}TeV, $\mathop {\mathgroup \symoperators tan}\nolimits \beta = 50$ and $\delta _{\rm  CKM} = 90^\circ $, where the hierarchy factor $\rho $ and $\phi _{A_U}$ are varied independently as shown above. The SM contributions alone for $\delta _{\rm  CKM} = 90^\circ $ are displayed by horizontal dashed lines.}}}{33}}
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\@writefile{lof}{\contentsline {figure}{\numberline {6}{\ignorespaces {\it  SUSY Higgs-penguin contributions to ${\cal  B} (\mathaccent "7016\relax {B}^0_s \to \mu ^+\mu ^-)$ and ${\cal  B} (\mathaccent "7016\relax {B}^0_d \to \tau ^+\tau ^-)$ versus the gluino phase ${\rm  arg}\, (m_{\mathaccent "707E\relax {g}})$, for $M_{\rm  SUSY} = 1$\nobreakspace  {}TeV, $M_{H^+} = 0.2$\nobreakspace  {}TeV, $\mathop {\mathgroup \symoperators tan}\nolimits \beta = 50$, and $\delta _{\rm  CKM} = 90^\circ $, where $\rho $ and $\phi _{A_U}$ are varied discretely.}}}{35}}
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\@writefile{lof}{\contentsline {figure}{\numberline {8}{\ignorespaces {\it  Numerical values for the CP asymmetries ${\cal  A}_{\rm  CP}^{(B^0_d \to \mu ^+_L\mu ^-_L )}$ and ${\cal  A}_{\rm  CP}^{(B^0_d \to \mu ^+_R\mu ^-_R )}$ as functions of the gluino phase ${\rm  arg}\, (m_{\mathaccent "707E\relax {g}})$, for $M_{\rm  SUSY} = 1$\nobreakspace  {}TeV, $M_{H^+} = 0.2$\nobreakspace  {}TeV, $\mathop {\mathgroup \symoperators tan}\nolimits \beta = 50$, and $\delta _{\rm  CKM} = 90^\circ $, where $\rho $ and $\phi _{A_U}$ are varied discretely. Also shown is the prediction for the CP asymmetries without including $B^0_d$-$\mathaccent "7016\relax {B}^0_d$ mixing.}}}{37}}
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\@writefile{lof}{\contentsline {figure}{\numberline {9}{\ignorespaces {\it  Numerical estimates of the CP asymmetries ${\cal  A}_{\rm  CP}^{(B^0_d \to \tau ^+_L\tau ^-_L )}$ and ${\cal  A}_{\rm  CP}^{(B^0_d \to \tau ^+_R\tau ^-_R )}$ versus the gluino phase ${\rm  arg}\, (m_{\mathaccent "707E\relax {g}})$, for $M_{\rm  SUSY} = 1$\nobreakspace  {}TeV, $M_{H^+} = 0.2$\nobreakspace  {}TeV, $\mathop {\mathgroup \symoperators tan}\nolimits \beta = 50$, and $\delta _{\rm  CKM} = 90^\circ $, where $\rho $ and $\phi _{A_U}$ take discrete values as shown above.}}}{38}}
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