Related Experiment Video
Updated: Jun 14, 2026

10:42
Preparing an Isotopically Pure 229Th Ion Beam for Studies of 229mTh
Published on: May 3, 2019
Bose-Einstein condensation of 84Sr.
Y N Martinez de Escobar1, P G Mickelson, M Yan
1Rice University, Department of Physics and Astronomy, Houston, Texas 77251, USA.
Physical Review Letters
|April 7, 2010
Summary
Researchers achieved Bose-Einstein condensation of strontium-84 atoms in an optical trap. This breakthrough enables the creation of large condensates, crucial for quantum simulations and atom optics.
Area of Science:
- Atomic, Molecular, and Optical Physics
- Quantum Gases
- Condensed Matter Physics
Background:
- Bose-Einstein condensation (BEC) is a state of matter formed by cooling fermions or bosons to near absolute zero.
- Strontium isotopes are promising candidates for BEC due to their unique atomic properties.
Purpose of the Study:
- To achieve Bose-Einstein condensation of the isotope Strontium-84 ((84)Sr).
- To investigate the feasibility of creating large condensates from a low-abundance isotope.
Main Methods:
- Utilizing laser cooling techniques on the narrow intercombination line of (84)Sr.
- Employing an optical dipole trap to confine the cooled atoms.
- Analyzing time-of-flight images to identify condensate formation.
Main Results:
- Successful Bose-Einstein condensation of (84)Sr was achieved.
- Large condensates with approximately 3 x 10^5 atoms were created.
- Condensation was indicated by the appearance of a low-velocity atomic component.
Conclusions:
- Bose-Einstein condensation of (84)Sr is feasible despite its low natural abundance.
- Efficient laser cooling and favorable scattering properties are key to creating large condensates.
- This work opens avenues for quantum applications using strontium BECs.
Related Concept Videos
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 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...
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:
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.
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;...
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...

