Jove
Visualize
Contact Us
JoVE
x logofacebook logolinkedin logoyoutube logo
ABOUT JoVE
OverviewLeadershipBlogJoVE Help Center
AUTHORS
Publishing ProcessEditorial BoardScope & PoliciesPeer ReviewFAQSubmit
LIBRARIANS
TestimonialsSubscriptionsAccessResourcesLibrary Advisory BoardFAQ
RESEARCH
JoVE JournalMethods CollectionsJoVE Encyclopedia of ExperimentsArchive
EDUCATION
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab ManualFaculty Resource CenterFaculty Site
Terms & Conditions of Use
Privacy Policy
Policies

Related Concept Videos

Types of Radioactivity03:23

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:
Nuclear Transmutation03:20

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...
Radioactivity and Nuclear Equations03:18

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...
Nuclear Stability03:18

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...
Nuclear Binding Energy02:13

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;...
Atomic Nuclei: Nuclear Spin State Population Distribution01:14

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.

You might also read

Related Articles

Articles linked to this work by shared authors, journal, and citation graph.

Sort by
Same author

Observation of high-energy neutrinos from the Galactic plane.

Science (New York, N.Y.)·2023
Same author

Evidence for neutrino emission from the nearby active galaxy NGC 1068.

Science (New York, N.Y.)·2022
Same author

Search for Unstable Sterile Neutrinos with the IceCube Neutrino Observatory.

Physical review letters·2022
Same author

Strong Constraints on Neutrino Nonstandard Interactions from TeV-Scale ν_{μ} Disappearance at IceCube.

Physical review letters·2022
Same author

Angular Analysis of D^{0}→π^{+}π^{-}μ^{+}μ^{-} and D^{0}→K^{+}K^{-}μ^{+}μ^{-} Decays and Search for CP Violation.

Physical review letters·2022
Same author

Search for Relativistic Magnetic Monopoles with Eight Years of IceCube Data.

Physical review letters·2022

Related Experiment Video

Updated: May 23, 2026

Setting Limits on Supersymmetry Using Simplified Models
07:46

Setting Limits on Supersymmetry Using Simplified Models

Published on: November 15, 2013

Search for lepton number violating decays B+ → π- μ+ μ+ and B+ → K- μ+ μ+.

R Aaij1, C Abellan Beteta, B Adeva

  • 1Nikhef National Institute for Subatomic Physics, Amsterdam, The Netherlands.

Physical Review Letters
|April 3, 2012
PubMed
Summary

Researchers searched for rare B+ decays violating lepton number, specifically B+ to K- or π- and two muons. No signal was observed, setting new world-leading limits on these rare particle physics processes.

More Related Videos

Preparing an Isotopically Pure 229Th Ion Beam for Studies of 229mTh
10:42

Preparing an Isotopically Pure 229Th Ion Beam for Studies of 229mTh

Published on: May 3, 2019

A Basic Positron Emission Tomography System Constructed to Locate a Radioactive Source in a Bi-dimensional Space
14:19

A Basic Positron Emission Tomography System Constructed to Locate a Radioactive Source in a Bi-dimensional Space

Published on: February 1, 2016

Related Experiment Videos

Last Updated: May 23, 2026

Setting Limits on Supersymmetry Using Simplified Models
07:46

Setting Limits on Supersymmetry Using Simplified Models

Published on: November 15, 2013

Preparing an Isotopically Pure 229Th Ion Beam for Studies of 229mTh
10:42

Preparing an Isotopically Pure 229Th Ion Beam for Studies of 229mTh

Published on: May 3, 2019

A Basic Positron Emission Tomography System Constructed to Locate a Radioactive Source in a Bi-dimensional Space
14:19

A Basic Positron Emission Tomography System Constructed to Locate a Radioactive Source in a Bi-dimensional Space

Published on: February 1, 2016

Area of Science:

  • Particle Physics
  • High Energy Physics
  • Standard Model Extensions

Background:

  • Lepton number violation is a key indicator of physics beyond the Standard Model.
  • The decay B+ → h- μ+ μ+ (where h- is K- or π-) is forbidden by the Standard Model but permitted in theories with Majorana neutrinos.

Purpose of the Study:

  • To search for the lepton number violating decay B+ → K- μ+ μ+ and B+ → π- μ+ μ+.
  • To set new, stringent limits on the branching fractions of these rare decays.
  • To probe new physics models, such as those incorporating Majorana neutrinos.

Main Methods:

  • Analysis of 36 fb⁻¹ of data collected by the LHCb detector.
  • Selection of candidate events for the B+ → K- μ+ μ+ and B+ → π- μ+ μ+ decay channels.
  • Statistical analysis to set upper limits on branching fractions at the 95% confidence level.

Main Results:

  • No significant signal was observed for either the B+ → K- μ+ μ+ or B+ → π- μ+ μ+ decay.
  • New upper limits on the branching fractions were established: B(B+ → K- μ+ μ+) < 5.4 × 10⁻⁸ and B(B+ → π- μ+ μ+) < 5.8 × 10⁻⁸.
  • These limits represent significant improvements over previous best limits, by factors of 40 and 30, respectively.

Conclusions:

  • The absence of signal provides strong constraints on new physics scenarios that predict lepton number violation.
  • The improved limits exclude a significant parameter space for models with Majorana neutrinos contributing to these decays.
  • This study highlights the power of LHCb in searching for rare and forbidden processes in particle physics.