Related Experiment Video
Updated: Jun 5, 2026

07:46
Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
Search for f(J)(2220) in radiative J/ψ decays
P del Amo Sanchez1, J P Lees, V Poireau
1Université de Savoie, CNRS/IN2P3, Annecy-Le-Vieux, France.
Physical Review Letters
|January 15, 2011
Summary
The BABAR experiment found no evidence for the f(J)(2220) resonance in J/ψ radiative decays. Upper limits were set on its production and decay rates, which are lower than previous measurements.
Area of Science:
- Particle Physics
- High-Energy Physics
- Quantum Chromodynamics
Background:
- The f(J)(2220) is a poorly understood meson resonance observed in J/ψ radiative decays.
- Previous experiments, like Mark III, reported evidence for this state, but its properties remain debated.
Purpose of the Study:
- To search for the f(J)(2220) resonance in radiative J/ψ decays (J/ψ→γf(J)(2220)).
- To investigate the f(J)(2220) decays into charged and neutral kaon pairs (K⁺K⁻ and K⁰SK⁰S).
- To set precise upper limits on the branching fractions for these processes.
Main Methods:
- Analysis of 460 fb⁻¹ of data collected by the BABAR detector at the PEP-II e⁺e⁻ collider.
- Reconstruction of J/ψ→γf(J)(2220) decays, with f(J)(2220) decaying into K⁺K⁻ and K⁰SK⁰S final states.
- Statistical analysis to set 90% confidence level upper limits on branching fractions.
Main Results:
- No significant evidence for the f(J)(2220) resonance was observed in the analyzed data.
- 90% confidence level upper limits on the product of branching fractions, B(J/ψ→γf(J)(2220)) × B(f(J)(2220)→K⁺K⁻ or K⁰SK⁰S), were established at the level of 10⁻⁵.
- These limits are below the central values reported by the Mark III experiment.
Conclusions:
- The absence of evidence for the f(J)(2220) in this high-statistics BABAR dataset challenges previous observations.
- The results provide stringent constraints on the existence and properties of the f(J)(2220) resonance.
- Further theoretical and experimental investigations are needed to clarify the nature of this particle or the discrepancy in observations.
Related Concept Videos
Atomic Absorption Spectroscopy: Radiation and Light Sources
Atomic absorption spectroscopy (AAS) relies on the Beer-Lambert law, which requires that the radiation source emits a narrow range of wavelengths to match the absorption characteristics of the analyte atom. The primary criteria for choosing an appropriate radiation source in AAS is to provide a precise and intense emission at specific wavelengths that will allow accurate detection of the analyte.
Two common narrow-range 'line' sources used in AAS are hollow-cathode lamps (HCLs) and...
Two common narrow-range 'line' sources used in AAS are hollow-cathode lamps (HCLs) and...
Atomic Nuclei: Nuclear Spin State Population Distribution
Near absolute zero temperatures, in the presence of a magnetic field, the majority of nuclei prefer the lower energy spin-up state to the higher energy spin-down state. As temperatures increase, the energy from thermal collisions distributes the spins more equally between the two states. The Boltzmann distribution equation gives the ratio of the number of spins predicted in the spin −½ (N−) and spin +½ (N+) states.
Atomic Radii and Effective Nuclear Charge
The elements in groups of the periodic table exhibit similar chemical behavior. This similarity occurs because the members of a group have the same number and distribution of electrons in their valence shells.
Atomic Nuclei: Larmor Precession Frequency
The earth's gravitational field produces a 'twisting force' perpendicular to the angular momentum of a spinning mass (such as a spinning top) that causes the mass to 'wobble' around the gravitational field axis in a phenomenon called precession. Similarly, the magnetic moment (μ) of a spinning nucleus precesses due to an external magnetic field directed along the z-axis. The precession of the magnetic moment vector about the magnetic field is called Larmor precession, and the angular frequency...
Isotopes and Radioisotopes
In the early 1900s, English chemist Frederick Soddy realized that an element could have atoms with different masses that were chemically indistinguishable. These different types are called isotopes — atoms of the same element that differ in mass. Isotopes differ in mass because they have different numbers of neutrons but are chemically identical because they have the same number of protons. Soddy was awarded the Nobel Prize in Chemistry in 1921 for this discovery.
An isotope containing more...
An isotope containing more...
Other Nuclides: 31P, 19F, 15N NMR
Many organic, inorganic, and biological molecules contain spin-half nuclei such as nitrogen-15, fluorine-19, and phosphorus-31. As a result, NMR studies of these nuclei have found extensive applications in chemical and biological research.
While fluorine-19 and phosphorous-31 have high natural abundances (100%) and positive gyromagnetic ratios, nitrogen-15 has a low natural abundance and a negative gyromagnetic ratio. However, nitrogen-15 is still preferred over nitrogen-14 (which has a high...
While fluorine-19 and phosphorous-31 have high natural abundances (100%) and positive gyromagnetic ratios, nitrogen-15 has a low natural abundance and a negative gyromagnetic ratio. However, nitrogen-15 is still preferred over nitrogen-14 (which has a high...
