B–Bbar oscillation
Neutral B meson oscillations (or
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Template:Rcatsh oscillations) are one of the manifestations of the neutral particle oscillation, a fundamental prediction of the Standard Model of particle physics. It is the phenomenon of B mesons changing (or oscillating) between their matter and antimatter forms before their decay. The [[strange B meson|
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Template:Rcatsh meson]] can exist as either a bound state of a strange antiquark and a bottom quark, or a strange quark and bottom antiquark. The oscillations in the neutral B sector are analogous to the phenomena that produce long and short-lived neutral kaons.
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Template:Rcatsh mixing was observed by the CDF experiment at Fermilab in 2006 and by LHCb at CERN in 2011 and 2021.
Excess of matter over antimatter
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The Standard Model predicts that regular matter [[strange B meson|
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Template:Rcatsh mesons]] are slightly favored in these oscillations over their antimatter counterpart, making strange B mesons of special interest to particle physicists. The observation of the
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Template:Rcatsh mixing phenomena led physicists to propose the construction of the so-named "B factories" in the early 1990s. They realized that a precise
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Template:Rcatsh oscillation measure could pin down the unitarity triangle and perhaps explain the excess of matter over antimatter in the universe. To this end construction began on two "B factories" in the late nineties, one at the Stanford Linear Accelerator Center (SLAC) in California and one at KEK in Japan.
These B factories, BaBar and Belle, were set at the [[Upsilon meson|
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Template:Rcatsh(4S)]] resonance which is just above the threshold for decay into two B mesons.
On 14 May 2010, physicists at the Fermi National Accelerator Laboratory reported that the oscillations decayed into matter 1% more often than into antimatter, which may help explain the abundance of matter over antimatter in the observed Universe.[1] However, more recent results at LHCb in 2011, 2012, and 2021 with larger data samples have demonstrated no significant deviation from the Standard Model prediction of very nearly zero asymmetry.[2][3][4]
See also
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References
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Further reading
- Script error: No such module "Citation/CS1". — paper describing the discovery of B-meson mixing by the ARGUS collaboration
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- Script error: No such module "citation/CS1". — announcement of the 5 sigma discovery