2<7 GeV2/c4)=(7.6±3.0-1.2 +0.9±3.0)×10-2 ns-1, ΔΓ(72<14 GeV2/c4)=(4.8 ±2.9-0.8+0.7±0.7)×10-2 ns-1, and ΔΓ(142<21 GeV2/c4)=(7.1±2.1-1.1 +0.9±0.6)×10-2 ns-1. Here, l=e or μ, but not both, and the errors are statistical, systematic, and theoretical. The method is sensitive primarily to B→ρlv decays with leptons in the energy range above 2.3 GeV. Averaging with the previously published CLEO results for B→ρlv, we obtain B(B0→ρ-l+v)=(2.57±0.29 -0.46+0.33±0.41)×10-4 and |Vub|=(3.25 ±0.14-0.29+0.21±0.55)×10-3. ©2000 The American Physical Society.
2<14 GeV2/c4)=(4.8 ±2.9-0.8+0.7±0.7)×10-2 ns-1, and ΔΓ(142<21 GeV2/c4)=(7.1±2.1-1.1 +0.9±0.6)×10-2 ns-1. Here, l=e or μ, but not both, and the errors are statistical, systematic, and theoretical. The method is sensitive primarily to B→ρlv decays with leptons in the energy range above 2.3 GeV. Averaging with the previously published CLEO results for B→ρlv, we obtain B(B0→ρ-l+v)=(2.57±0.29 -0.46+0.33±0.41)×10-4 and |Vub|=(3.25 ±0.14-0.29+0.21±0.55)×10-3. ©2000 The American Physical Society.
2<21 GeV2/c4)=(7.1±2.1-1.1 +0.9±0.6)×10-2 ns-1. Here, l=e or μ, but not both, and the errors are statistical, systematic, and theoretical. The method is sensitive primarily to B→ρlv decays with leptons in the energy range above 2.3 GeV. Averaging with the previously published CLEO results for B→ρlv, we obtain B(B0→ρ-l+v)=(2.57±0.29 -0.46+0.33±0.41)×10-4 and |Vub|=(3.25 ±0.14-0.29+0.21±0.55)×10-3. ©2000 The American Physical Society.