Related Experiment Video
Updated: Aug 5, 2026

07:46
Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
Search for the rare leptonic decay B+-->mu(+)nu(mu)
B Aubert1, R Barate, D Boutigny
1Laboratoire de Physique des Particules, F-74941 Annecy-le-Vieux, France.
Physical Review Letters
|July 13, 2004
Summary
Researchers searched for the rare B+ to muon neutrino decay using BABAR experiment data. No significant signal was found, establishing an upper limit for this rare B+ meson decay.
Area of Science:
- Particle Physics
- High Energy Physics
- Experimental Physics
Background:
- Rare B+ meson decays offer insights into fundamental particle physics.
- Leptonic decays, such as B+ to muon neutrino, are particularly sensitive to new physics beyond the Standard Model.
- Previous searches have constrained the branching fractions of such rare decays.
Purpose of the Study:
- To search for the rare leptonic decay B+ --> mu(+)nu(mu).
- To set an upper limit on the branching fraction of this decay using experimental data.
- To probe for potential new physics contributions to B+ meson decays.
Main Methods:
- Utilized data collected by the BABAR experiment at the PEP-II storage ring.
- Analyzed a sample of 88.4 x 10^6 BBbar meson pairs collected at the Upsilon(4S) resonance.
- Employed analysis techniques to identify and reconstruct the B+ --> mu(+)nu(mu) decay signature.
Main Results:
- No significant evidence for the B+ --> mu(+)nu(mu) signal was observed.
- An upper limit on the branching fraction was established at B(B+ --> mu(+)nu(mu)) < 6.6 x 10^-6.
- The result is reported at the 90% confidence level.
Conclusions:
- The absence of a signal places stringent constraints on the branching fraction of this rare decay.
- The findings contribute to the ongoing effort to test the Standard Model of particle physics.
- This measurement helps to limit the parameter space for potential new theoretical models.
Related Concept Videos
Electron Configuration of Multielectron Atoms
The alkali metal sodium (atomic number 11) has one more electron than the neon atom. This electron must go into the lowest-energy subshell available, the 3s orbital, giving a 1s22s22p63s1 configuration. The electrons occupying the outermost shell orbital(s) (highest value of n) are called valence electrons, and those occupying the inner shell orbitals are called core electrons. Since the core electron shells correspond to noble gas electron configurations, we can abbreviate electron...
Radioactivity and Nuclear Equations
Nuclear chemistry is the study of reactions that involve changes in nuclear structure. The nucleus of an atom is composed of protons and, except for hydrogen, neutrons. The number of protons in the nucleus is called the atomic number (Z) of the element, and the sum of the number of protons and the number of neutrons is the mass number (A). Atoms with the same atomic number but different mass numbers are isotopes of the same element.
A nuclide of an element has a specific number of protons and...
A nuclide of an element has a specific number of protons and...
Types of Radioactivity
The most common types of radioactivity are α decay, β decay, γ decay, neutron emission, and electron capture.
Alpha (α) decay is the emission of an α particle from the nucleus. For example, polonium-210 undergoes α decay:
Alpha (α) decay is the emission of an α particle from the nucleus. For example, polonium-210 undergoes α decay:
Nuclear Stability
Protons and neutrons, collectively called nucleons, are packed together tightly in a nucleus. With a radius of about 10−15 meters, a nucleus is quite small compared to the radius of the entire atom, which is about 10−10 meters. Nuclei are extremely dense compared to bulk matter, averaging 1.8 × 1014 grams per cubic centimeter. If the earth’s density were equal to the average nuclear density, the earth’s radius would be only about 200 meters.
To hold positively charged protons together in the...
To hold positively charged protons together in the...
Nuclear Binding Energy
The difference between the calculated and experimentally measured masses is known as the mass defect of the atom. In the case of helium-4, the mass defect indicates a “loss” in mass of 4.0331 amu – 4.0026 amu = 0.0305 amu. The loss in mass accompanying the formation of an atom from protons, neutrons, and electrons is due to the conversion of that mass into energy that is evolved as the atom forms. The nuclear binding energy is the energy produced when the atoms’ nucleons are bound together;...
Nuclear Transmutation
Nuclear transmutation is the conversion of one nuclide into another. It can occur by the radioactive decay of a nucleus, or the reaction of a nucleus with another particle. The first manmade nucleus was produced in Ernest Rutherford’s laboratory in 1919 by a transmutation reaction, the bombardment of one type of nuclei with other nuclei or with neutrons. Rutherford bombarded nitrogen-14 atoms with high-speed α particles from a natural radioactive isotope of radium and observed protons being...

