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The Decays of $B^{+}\to{\bar{D}^0}+D^{+}_{sJ}(2S)$ and $B^{+}\to\bar{D}^{0}+D^{+}_{sJ}(1D)$ PDF

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Preview The Decays of $B^{+}\to{\bar{D}^0}+D^{+}_{sJ}(2S)$ and $B^{+}\to\bar{D}^{0}+D^{+}_{sJ}(1D)$

The Decays of B+ D¯0 + D+ (2S) and B+ D¯0 + D+ (1D) sJ sJ → → Guo-Li Wang∗, Jin-Mei Zhang and Zhi-Hui Wang Department of Physics, Harbin Institute of Technology, Harbin 150001,China 0 1 0 2 n a ABSTRACT J 3 1 We analyzed the decays of B+ D¯0 + D+(2S) and B+ D¯0 + D+(1D) by naive fac- ] → sJ → sJ h p torization method and model dependent calculation based on the Bethe-Salpeter method, - p the branching ratios are Br(D¯0D+(2S)) = (0.72 0.12)% and Br(D¯0D+(1D)) = (0.027 e sJ ± sJ ± h [ 0.007)%. The branching ratio of decay B+ D¯0D+(2S) D¯0D0K+ consist with the data → sJ → 1 v of Belle Collaboration, so we conclude that the new state D+(2700) is the first excited state sJ 5 3 D+(2S). 0 sJ 2 . 1 0 0 1 : v i X r a ∗gl [email protected] 1 BABAR Collaboration reported the observation of a new charmed meson called D+(2690) with a sJ mass 2688 4 3 MeV and with a broad width Γ = 112 7 36 MeV [1], Belle Collaboration also ± ± ± ± reported a charmed state D+(2700), M = 2715 11+11 MeV with width Γ = 115 20+36 MeV [2], later sJ ± −14 ± −32 modified to M = 2708 9+11 MeV and Γ = 108 23+36 MeV [3]. Most authors believe that these two ± −10 ± −31 states should beone state, and the most possiblecandidate is the 2S or the S D (2 3S 1 3D ) mixing 1 1 − − − cs¯1 state [4, 5, 6, 7, 8, 9, 10, 11]. Recently, we have analyzed the decays of the D+(2S) and D+(1D), we concluded that one can not sJ sJ distinguish them from their decays, because they have the similar decay channels and the corresponding decay widths are comparable [12]. In this paper, we give the calculations of the decays B+ D¯0 + → D+(2S) and B+ D¯0 +D+(1D), we find that we can separate them, and according to the current sJ → sJ experimental data of Belle Collaboration, we conclude that the new state D+(2700) is the first excited sJ state D+(2S). These channels have also been considered in literatures, for example, Close et al [4, 23] sJ give branching ratios and possible mixing of 2S and 1D; Colangelo et al [7] assume the new state is the 2S state, and extract the decay constant. The decay amplitude for B+ D¯0+D+ can be described in the naive factorization approach: → sJ G T = FV V a D+ J 0 D¯0 Jµ B+ , (1) cs cb 1 µ √2 h sJ| | ih | | i where the CKM matrix element V = 0.97334 and V = 0.0415 [13], since we focus on the difference cs cb between D+(2S) and D+(1D), not on the careful study, we have chosen a = c +1c = 1, where c and sJ sJ 1 1 3 2 1 c are the Wilson coefficients [14]. We also delete other higher order contributions like the contributions 2 from penguin operators. And D+ J 0 = iF∗M ǫλ , (2) h sJ| µ| i V Ds+J µ F and ǫλ are the decay constant and polarization vector of the meson D+, respectively. V µ sJ We have solved the exact instantaneous Bethe-Salpeter equations [15] (or the Salpeter equations [16]) − − for1 states, thegeneral formfor therelativistic Salpeter wave function of vector 1 state can bewritten as [17, 18]: ϕλ1−(q⊥) = q⊥·ǫλ⊥(cid:20)f1(q⊥)+ M6P f2(q⊥)+ 6Mq⊥f3(q⊥)+ 6PM6q2⊥f4(q⊥)(cid:21)+M6ǫλ⊥f5(q⊥) 1 +ǫλ⊥Pf6(q⊥)+(q⊥ǫλ⊥ q⊥ ǫλ⊥)f7(q⊥)+ (Pǫλ⊥q⊥ Pq⊥ ǫλ⊥)f8(q⊥), (3) 6 6 6 6 − · M 6 6 6 −6 · 1 wherethe P, q andǫλ arethe momentum, relative innermomentum and polarization vector of thevector ⊥ meson, respectively; fi(q⊥)is the functionof q⊥2, andwe have usedthenotation q⊥µ qµ (P q/M2)Pµ − ≡ − · (which is (0, ~q) in the center of mass system). The 8 wave functions f are not independent, there are only 4 independent wave functions [18], and i we have the relations q⊥2f3(q⊥)+M2f5(q⊥) (m1m2 ω1ω2+q⊥2) f5(q⊥)M( m1m2+ω1ω2+q⊥2) f1(q⊥)= (cid:2) M(m +(cid:3)m )q2 − , f7(q⊥)= (−m m )q2 , 1 2 ⊥ 1 2 ⊥ − q⊥2f4(q⊥)+M2f6(q⊥) (m1ω2 m2ω1) f6(q⊥)M(m1ω2 m2ω1) f2(q⊥)= (cid:2)− M(ω +ω (cid:3))q2 − , f8(q⊥)= (ω ω )q−2 . 1 2 ⊥ 1 2 ⊥ − − In our method, the S D mixing automatically exist in the wave function of 1 state, because we − give the whole wave function Eq. (3) which is JP = 1−, but some of the wave function are S wave, some are D wave, for example, see Figure 1-3, we show wave functions. One can see that, for 1S and 2S, the wave function f and f are dominate, and they are S wave, but there is little D wave mixing in these 5 6 two states which come from the terms f and f . But for the third state, we labeled as 1D state, the 3 4 terms f and f are dominate, but these two terms are not pure D wave, they will give contribute as a 3 4 S wave [17]. So we conclude that the 1S and 2S states are S wave dominate states, mixed with a little D wave (come from the terms f and f ), while the 1D state is a D wave dominate state (f and f ), 3 4 3 4 mixed with a valuable part of S wave (still come from the terms f and f ). 3 4 − For cs¯vector 1 state, our mass prediction for the first radial excited 2S state is 2673 MeV, and for 1D, our result is 2718 MeV [18], so there are two states around 2700 MeV. InRef. [18],weonlygivetheleadingordercalculationfordecayconstant,whichisF = 4√N dq~ f (~q), V c (2π)3 5 R the whole equation should be dq~ ~q2f 3 F = 4 N (f ), (4) V cZ (2π)3 5− 3M2 p and our results of the decay constants for vector cs¯system are: F (1S) = 353 21 MeV, V ± F (2S) = 295 13 MeV, V ± F (1D) = 57.1 5.1 MeV. V ± Where the uncertainties are given by varying all the input parameters simultaneously within 5% of ± the central values in our model, and we will calculate all the uncertainties this way in this letter. The 2 7 ) 6 2 2 2 - V q f (|q|)/M 3 e G 2 2 ( 5 q f4(|q|)/M e at f5(|q|) t s 4 S -f6(|q|) 1 r o f 3 s n o nti 2 c u f e v 1 a w 0 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 |q| GeV ∗ Figure 1: wave functions of D (1S). s 10 ) -2 V 8 q2f (|q|)/M2 e 3 G 2 2 ( q f (|q|)/M 4 e t 6 a f (|q|) t 5 s S -f (|q|) 6 2 r 4 o f s n o cti 2 n u f e v a 0 w -2 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 |q| GeV ∗ Figure 2: wave functions of D (2S). s 3 6 ) 2 2 2 - V q f (|q|)/M e 3 G 5 2 2 ( q f4(|q|)/M e t a f (|q|) st 4 5 D -f (|q|) 6 1 r o f 3 s n o ti c n 2 u f e v a 1 w 0 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 4.0 |q| GeV ∗ Figure 3: wave functions of D (1D). s center values of S waves are little smaller than the estimates in Ref. [18], where F (1S) = 375 24 MeV V ± and F (2S) = 312 17 MeV, but the value of D wave decay constant is much smaller than the predict V ± in Ref. [18] where we did not shown it, this is because we should not ignore the contribution from the term of f when consider a D wave state. Our estimate of F (1S) = 353 23 MeV is close to the 3 V ± newer result FD∗ = 268 290 MeV by Choi [19]. Our estimate of FV(2S) = 312 17 MeV is a little s ∼ ± larger than the estimate F (2S) = 243 41 MeV in Ref. [7], where they extracted it from the decay V ± B+ D¯0+D+(2700) assuming the new state D+(2700) is the first radial excited state D+(2S). → sJ sJ sJ According to the Mandelstam formalism [20], at the leading order, the transition amplitude for B+ D¯0 can be written as [21]: → dq~ m P D¯0 Jµ B+ = Tr ϕ¯++(~q u ~r)6 ϕ++(~q)γµ(1 γ ) , (5) h | | i Z (2π)3 (cid:20) D¯0 − mc+mu M B+ − 5 (cid:21) where~r is the recoil three dimensional momentum of the final state D¯0 meson, ϕ++ is called the positive energy wave function, and ϕ¯++ = γ (ϕ++)+γ . 0 0 D¯0 D¯0 The wave function forms for pseudoscalar B+ and D¯0 are similar, for example, the wave function for B+ can be written as [22] → M → → m +m ϕ++(q) = B+ ϕ (q)+ϕ (q) u b B+ 2 (cid:18) 1 2 ωu+ωb (cid:19) 4 ω +ω ~q(m m ) ~qγ (ω +ω ) u b +γ 6 u − b + 6 0 u b γ , (6) ×(cid:20)m +m 0 − m ω +m ω (m ω +m ω )(cid:21) 5 u b b u u b b u u b where ω = m2 +~q2 and ω = m2+~q2; ϕ (~q), ϕ (~q) are the radial part wave functions, and their u u b b 1 2 q p − numerical values can be obtained by solving the full Salpter equation of 0 state [22]. The decay width is: 1 p~ Γ = | f2| T 2 8π M2 | | B 1 p~ G2V2V2 = | f2| F cs bcF2M2 X, (7) 8π M2 2 V f2 B where p~ and M are the three dimensional momentum and mass of the final new state D∗+. M2 f2 f2 sJ f2 come from the definition of decay constant in Eq.(2), but the square of polarization vector and transition amplitude of Eq.(5) are symbolized as X. So our result are: Γ(B+ D¯0D∗+(2S)) = F2(2S) (3.50 0.38) 10−14 GeV, (8) s V → × ± × Γ(B+ D¯0D∗+(1D)) = F2(1D) (3.25 0.30) 10−14 GeV. (9) s V → × ± × If we ignore the mass difference between D∗+(2S) and D∗+(1D), and use 2700 MeV as input, the results s s become Γ(B+ D¯0D∗+(2S)) = F2(2S) (3.36 0.25) 10−14 GeV, (10) s V → × ± × Γ(B+ D¯0D∗+(1D)) = F2(1D) (3.36 0.25) 10−14 GeV. (11) s V → × ± × So the difference between this two channel mainly come from the difference of decay constants. Then our predictions of branching ratios are: Br(B+ D¯0D∗+(2S)) =(0.72 0.12)%, (12) s → ± Br(B+ D¯0D∗+(1D)) = (0.027 0.007)%. (13) s → ± In Ref. [12], we have calculated the main decay channels of D+(2S) and D+(1D), and we have the sJ sJ following estimates: Br(D+(2S) D0K+) = 0.20 0.03 sJ → ± 5 and Br(D+(1D) D0K+) = 0.32 0.04, sJ → ± so we obtain: Br(B+ D¯0D+(2S)) Br(D+(2S) D0K+) = (1.4 0.5) 10−3 (14) → sJ × sJ → ± × and Br(B+ D¯0D+(1D)) Br(D+(1D) D0K+) = (0.9 0.3) 10−4. (15) → sJ × sJ → ± × Our estimate of Br(D+(2S) D0K+) 0.20 is larger than than the estimate 0.11 in Ref. [4] and sJ → ≃ the estimate 0.05 in Ref. [5], if we use their value as input, we will obtain a smaller value of Br(B+ → D¯0D+(2S)) Br(D+(2S) D0K+). But our estimate of Br(D+(1D) D0K+) 0.32 consist with sJ × sJ → sJ → ≃ the value 0.34 in Ref. [5]. One can also see that, the final branching ratios depend strongly on the decay constants, but at this time few papers have calculated the values of decay constants for D+(2S) and sJ D+(1D). In Ref. [7], they assumed that the new state D+(2700) is D+(2S), and they extracted decay sJ sJ sJ constant of D+(2S): F = 243 41 MeV. sJ Ds+J(2S) ± The Belle Collaboration have the data [3, 13] Br(B+ D¯0D+(2700)) Br(D+(2700) D0K+) = (1.13 +0.26) 10−3. → sJ × sJ → −0.36 × Because we only calculated the decay widths of six main channels for D+(2S) (D+(1D)), and based sJ sJ on the summed width of these six channels, not full width, we give a relative larger branching ratio Br(D+(2S) D0K+) and Br(D+(1D) D0K+), the real branching ratios should be smaller than sJ → sJ → our estimates, so our estimate of B+ decay to D+(2S) is close to the data, while the estimate of B+ sJ decay to D+(1D) is much smaller than the data, then we can draw a conclusion that the new state sJ D+(2700) is D+(2S). sJ sJ We have another method to estimate the branching ratio, because the mass of B+ is much heavier than the mass of D¯0, and the mass of D+(2700) is close to the mass of D∗+, as a rough estimate, we sJ s ignore the mass difference of D+(2700) and D∗+(2112), from Eq.(1) and Eq.(2), then we have sJ s Br(B+ D¯0D+(2S)) F2(2S) → sJ V , (16) Br(B+ D¯0D∗+(1S)) ≃ F2(1S) s V → and from Particle Data Group [13], the branching ratio of B+ D¯0+D+(1S): → sJ Br(B+ D¯0D∗+(1S)) = (7.8 1.6) 10−3. s → ± × 6 So we have: F2(2S) Br(B+ D¯0D∗+(2S)) V (7.8 1.6) 10−3 (5.4 1.7) 10−3, (17) → s ≃ F2(1S) × ± × ≃ ± × V F2(1D) Br(B+ D¯0D∗+(1D)) V (7.8 1.6) 10−3 (2.0 1.0) 10−4. (18) → s ≃ F2(1S) × ± × ≃ ± × V This rough estimate results are very close to our calculations (Eq.(12) and Eq.(13)), so we have the same conclusion that D+(2700) is D+(2S). sJ sJ In Ref. [12], we estimate the full widths of D+(2S) and D+(1D) by six main decay channels, the sJ sJ estimated full widths are 46.4 6.2 MeV for D+(2S), 73.0 10.4 MeV for D+(1D), comparing with ± sJ ± sJ experimental data, Γ = 112 7 36 MeV for D+(2690) and Γ = 108 23+36 MeV for D+(2700), there ± ± sJ ± −31 sJ is still the possible that there are two states around 2700 MeV, one is the S wave dominate D+(2S), the sJ other is D wave dominate D+(1D). sJ As summary, from the decays B+ D¯0+D+(2S) and B+ D¯0+D+(1D), we conclude that the → sJ → sJ new state D+(2700) is the first radial excited state D+(2S), and there may exist another state around sJ sJ 2700, D+(1D), with a mass around 2718 MeV, and a width 73.0 10.4 MeV. sJ ± Acknowledgements This work was supportedin partby theNational Natural Science Foundation of China(NSFC) under Grant No. 10875032, and in part by SRF for ROCS, SEM. References [1] BABAR Collaboration, B. Aubert et al., Phys. Rev. Lett. 97, (2006) 222001. [2] Belle Collaboration, K. Abe et al., e-Print: hep-ex/0608031. [3] Belle Collaboration, J. Brodzicka et al., Phys. Rev. Lett. 100, (2008) 092001. [4] F. E. Close, C. E. Thomas, Olga Lakhina and Eric S. Swanson, Phys. Lett. B647 (2007) 159. [5] Bo Zhang, Xiang Liu, Wei-Zhen Deng and Shi-Lin Zhu, Eur. Phys. J. C50, (2007) 617. [6] J. L. Rosner, J. Phys. G34, (2007) S127. [7] P. Colangelo, F. De Fazio, S. Nicotri and M. Rizzi, Phys. Rev. D77, (2008) 014012. [8] Takayuki Matsuki, Toshiyuki, Kazutaka Sudoh, Eur. Phys. J. A31, (2007) 701. 7 [9] De-Min Li, Bing Ma, Yun-Hu Liu, Eur. Phys. J. C51, (2007) 359. [10] Xian-Hui Zhong, Qiang Zhao, Phys. Rev. D78, (2008) 014029. [11] Xue-Qian Li, Xiang Liu, Zheng-Tao Wei, e-Print: arXiv: 0808.2587. [12] Guo-Li Wang, Jin-Mei Zhang and Zhi-Hui Wang, submited. [13] Particle Data Group, Phys. Lett. B667 (2008) 1. [14] Matthias Neubert, Berthold Stech, Adv. Ser. Direct. High Energy Phys. 15 (1998) 294. [15] E. E. Salpeter and H. A. Bethe, Phys. Rev. 84, (1951) 1232. [16] E. E. Salpeter, Phys. Rev. 87, (1952) 328. [17] Chao-Hsi Chang, Jiao-Kai Chen, Xue-Qian Li and Guo-Li Wang, Commun. Theor. Phys. 43 (2005) 113. [18] Guo-Li Wang, Phys. Lett. B633 (2006) 492. [19] Ho-Meoyng Choi, Phys. Rev. D75 (2007) 073016. [20] S. Mandelstam, Proc. R. Soc. London 233, 248 (1955). [21] Chao-Hsi Chang, C. S. Kim, Guo-Li Wang, Phys. Lett. B623 (2005) 218. [22] C. S. Kim and Guo-Li Wang, Phys. Lett. B584 (2004) 285. [23] F. E. Close and E. S. Swanson, Phys. Rev. D72 (2005) 094004. 8

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