27.04.2015 Views

download report - Sapienza

download report - Sapienza

download report - Sapienza

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

Scientific Report 2007-2009<br />

Particle physics<br />

P13. Observation of direct CP violation in B meson decays.<br />

Matter and antimatter were produced in equal amount<br />

according to the Big Bang theories on the origin of the<br />

Universe, but our experience tells us that the Universe is<br />

clearly matter-dominated. According to A.D. Sakharov<br />

one of the key element to understand the disappearance<br />

of antimatter is the nonconservation of the charge-parity<br />

(CP ) symmetry in the fundamental forces governing the<br />

interactions of particles.<br />

So far, two types of CP violation have been observed<br />

in the neutral K meson (K 0 ) and B meson (B 0 ) systems:<br />

CP violation involving the flavour mixing between the<br />

meson and its antiparticle ( B 0 and ¯B 0 ) and direct CP<br />

violation in the decays of each meson. Direct CP violation<br />

effects are explained by the quantum interference<br />

of (at least) two competiting decay amplitudes. This interference<br />

has opposite sign for B 0 with respect to the<br />

¯B 0 decays, resulting in a non-null difference of the decay<br />

rate for the B 0 and the ¯B 0 .<br />

Events / 30 MeV<br />

400<br />

200<br />

0<br />

-0.1 0 0.1<br />

∆E (GeV)<br />

Figure 2: ∆E observable (equivalent to the invariant mass<br />

of the decay products) for the decays B 0 → K + π − (blue)<br />

and for ¯B 0 → K − π + (red). The direct CP asymmetry is<br />

given by the clear unbalance in the number of events.<br />

Figure 1: Quartz bar of the detector for internally reflected<br />

Cerenkov light of the BaBar experiment<br />

In the last years the BaBar group of Roma was part<br />

of a large international collaboration that operated a detector<br />

at the Stanford Linear Accelerator Center (California)<br />

where a copious source of B meson was available<br />

at the PEP-II e + e − collider. The group was involved<br />

in data analysis with a special focus to rare decays of<br />

the B meson into light mesons. Combinations of rates<br />

measurements [1] of such decays are very sensitive to the<br />

CP parameters of the Standard Model (SM) of particle<br />

interaction.<br />

One interesting channel is the B decay into the twobody<br />

final state K ± π ∓ [2]. The identification of the<br />

mass of the final state particles was possible through an<br />

innovative apparatus able to detect the Cerenkov light<br />

emitted by the two particles crossing a quartz bar (shown<br />

in Fig.1). By measuring the ultraviolet light emission angles,<br />

kaon and pion were identified with very high precision.<br />

A careful analysis of the collected data led the<br />

Roma group to publish the first evidence of direct CP<br />

violation in the B meson system. This was in fact possible<br />

by counting the B 0 → K + π − decays versus the<br />

¯B 0 → K − π + decays and finding a clear difference between<br />

the two samples (as shown in Fig.2).<br />

The observed CP violation effects are large in the<br />

B 0 meson system and they are consistent with the SM<br />

prediction, which has a unique source of CP violation.<br />

The theoretical mechanism generating such effect is<br />

known as the Cabibbo-Kobayashi-Maskawa model:<br />

the 2008 Nobel Prize in Physics was awarded to M.<br />

Kobayashi and T. Maskawa for this theory. Nevertheless<br />

the SM CP violation is too small to account for the<br />

matter-dominated Universe. Further investigations of<br />

such effects in several decays channels are therefore<br />

necessary to explain such dominance of matter. They<br />

have been started by the Roma BaBar group [3,4] but<br />

they may become conclusive only in future experiments<br />

with larger B meson data sets.<br />

References<br />

1 B. Aubert et al., Phys. Rev. D 76, 091102 (2007)<br />

2 B. Aubert et al., Phys. Rev. Lett. 99, 021603 (2007).<br />

3 B. Aubert et al., Phys. Rev. Lett. 99, 161802 (2007).<br />

4 B. Aubert et al., Phys. Rev. D 78, 012004 (2008).<br />

Authors<br />

F. Bellini, G. Cavoto 1 , D. del Re, E. Di Marco, R. Faccini,<br />

F. Ferrarotto 1 , F.Ferroni, M. Gaspero, L. Li Gioi, M. A.<br />

Mazzoni 1 , S. Morganti 1 , G. Piredda 1 , F. Renga 1 , C. Voena 1<br />

http://babar.roma1.infn.it/roma<br />

<strong>Sapienza</strong> Università di Roma 120 Dipartimento di Fisica

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!