Search for D0-D0bar Mixing

We report on a search for D0-D0bar mixing made by a study of the `wrong-sign' process D0 -> K+pi-. The data come from an integrated luminosity of e+e- collisions at sqrt{s} of about 10 GeV consisting of 9.0 1/fb recorded with the CLEO-II.V detector. We measure the time-integrated rate of the...

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description We report on a search for D0-D0bar mixing made by a study of the `wrong-sign' process D0 -> K+pi-. The data come from an integrated luminosity of e+e- collisions at sqrt{s} of about 10 GeV consisting of 9.0 1/fb recorded with the CLEO-II.V detector. We measure the time-integrated rate of the `wrong-sign' process D0 -> K+pi-, relative to that of the Cabibbo-favored process D0bar -> K+pi-, to be R_ws=(0.34+-0.07+-0.06)%. We study that rate as a function of the decay time of the D0, to distinguish the rate of direct doubly-Cabibbo-suppressed decay from D0-D0bar mixing. The amplitudes that describe D0-D0bar mixing, x' and y', are consistent with zero. The one-dimensional limits, at the 95% C.L., that we determine are (1/2)x'^2
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The data come from an integrated luminosity of e+e- collisions at sqrt{s} of about 10 GeV consisting of 9.0 1/fb recorded with the CLEO-II.V detector. We measure the time-integrated rate of the `wrong-sign' process D0 -&gt; K+pi-, relative to that of the Cabibbo-favored process D0bar -&gt; K+pi-, to be R_ws=(0.34+-0.07+-0.06)%. We study that rate as a function of the decay time of the D0, to distinguish the rate of direct doubly-Cabibbo-suppressed decay from D0-D0bar mixing. The amplitudes that describe D0-D0bar mixing, x' and y', are consistent with zero. The one-dimensional limits, at the 95% C.L., that we determine are (1/2)x'^2&lt;0.05%, and -5.9% &lt; y' &lt; 0.3%. 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The data come from an integrated luminosity of e+e- collisions at sqrt{s} of about 10 GeV consisting of 9.0 1/fb recorded with the CLEO-II.V detector. We measure the time-integrated rate of the `wrong-sign' process D0 -&gt; K+pi-, relative to that of the Cabibbo-favored process D0bar -&gt; K+pi-, to be R_ws=(0.34+-0.07+-0.06)%. We study that rate as a function of the decay time of the D0, to distinguish the rate of direct doubly-Cabibbo-suppressed decay from D0-D0bar mixing. The amplitudes that describe D0-D0bar mixing, x' and y', are consistent with zero. The one-dimensional limits, at the 95% C.L., that we determine are (1/2)x'^2&lt;0.05%, and -5.9% &lt; y' &lt; 0.3%. All results are preliminary.</abstract><doi>10.48550/arxiv.hep-ex/9909028</doi><oa>free_for_read</oa></addata></record>
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title Search for D0-D0bar Mixing
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