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2011 QCD and High Energy Interactions - Rencontres de Moriond ...

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2 Estimating the hadronic matrix elements of the HQE<br />

Within HQE, the total semileptonic rate as well as the differential distributions are represented<br />

in terms of an expansion of the form<br />

dΓ = dΓ0 +<br />

<br />

+dΓ5<br />

Λ<strong>QCD</strong><br />

a0<br />

2<br />

dΓ2 +<br />

mb<br />

5 Λ<strong>QCD</strong><br />

mb<br />

+ a2<br />

Λ<strong>QCD</strong><br />

3<br />

dΓ3 +<br />

Λ<strong>QCD</strong><br />

mb mb<br />

3 <br />

2<br />

Λ<strong>QCD</strong> Λ<strong>QCD</strong><br />

mb<br />

mc<br />

4<br />

dΓ4<br />

+ ... + dΓ7<br />

3 4 Λ<strong>QCD</strong> Λ<strong>QCD</strong><br />

The coefficients dΓi are themselves functions of mc/mb which are – up to logarithms of mc<br />

– regular in the limit mc → 0, <strong>and</strong> which have an expansion in αs(mb). Furthermore, the<br />

dΓi <strong>de</strong>pend on non-perturbative parameters corresponding to matrix elements of increasing<br />

dimension.<br />

The relevant hadronic matrix elements are<br />

for dΓ2 <strong>and</strong><br />

2MHµ 2 π = −〈H(v)| ¯ Qv(iD) 2 Qv|H(v)〉 : Kinetic <strong>Energy</strong> (2)<br />

2MHµ 2 G = 〈H(v)| ¯ Qvσµν(iD µ )(iD ν )Qv|H(v)〉 : Chromomagnetic Moment (3)<br />

2MHρ 3 D = −〈H(v)| ¯ Qv(iDµ)(ivD)(iD µ )Qv|H(v)〉 : Darwin Term (4)<br />

2MHρ 3 LS = 〈H(v)| ¯ Qvσµν(iD µ )(ivD)(iD ν )Qv|H(v)〉 : Spin-Orbit Term (5)<br />

for dΓ3.<br />

Going to higher or<strong>de</strong>rs one faces a proliferation of the number of in<strong>de</strong>pen<strong>de</strong>nt matrix elements.<br />

At or<strong>de</strong>r 1/m4 b we have already nine matrix elements, at or<strong>de</strong>r 1/m5b this increases to<br />

18, <strong>and</strong> at 1/m6 b there will be already 72 in<strong>de</strong>pen<strong>de</strong>nt non-perturbative parameters.<br />

Obviously these parameters cannot be <strong>de</strong>termined from experiment any more, <strong>and</strong> hence we<br />

have to find a way to estimate them theoretically. To this end, we <strong>de</strong>fine a way for such an<br />

estimate based on a simple asumption which, however, can be systematically refined.<br />

The higher or<strong>de</strong>r matrix elements can all be expressed in the form<br />

〈B| ¯ b iDµ1 iDµ2 · · · iDµn Γ b(0)|B〉, (6)<br />

where Γ <strong>de</strong>notes an arbitrary Dirac matrix. The representation is obtained by splitting the full<br />

chain iDµ1iDµ2 · · · iDµn into A=iDµ1 iDµ2 · · · iDµk <strong>and</strong> C =iDµk+1iDµk+2 · · · iDµn.<br />

In or<strong>de</strong>r to discuss the i<strong>de</strong>a of the method we shall first assume that the <strong>de</strong>rivatives in A<br />

<strong>and</strong> C are all spatial <strong>de</strong>rivatives. In the following we show the intermediate state represenation<br />

〈B| ¯b AC Γ b(0)|B〉 = 1 <br />

〈B|<br />

2MB n<br />

¯bAb(0)|n〉 · 〈n| ¯b C Γ b(0)|B〉, (7)<br />

where we have assumed the B mesons to be static <strong>and</strong> at rest, |B〉 = |B(p=(MB,0))〉, <strong>and</strong> |n〉<br />

are the single-b hadronic states with vanishing spatial momentum.<br />

Eq. (7) can be proven based on the operator product expansion. We introduce a ficticious<br />

heavy quark Q which will be treated as static, <strong>and</strong> consi<strong>de</strong>r a correlator at vanishing spatial<br />

momentum transfer q<br />

<br />

TAC(q0) = d 4 x e iq0x0<br />

<br />

〈B|iT ¯bAQ(x) QCΓb(0) ¯ |B〉. (8)<br />

We shall use the static limit for both b <strong>and</strong> Q, <strong>and</strong> hence introduce the ‘rephased’ fields<br />

˜Q(x) = e imQq0x0 Q(x) <strong>and</strong> likewise for b, <strong>and</strong> omit til<strong>de</strong> in them in what follows. The form of<br />

mb<br />

mc<br />

(1)

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