RSS icon
Twitter icon
Facebook icon
Vimeo icon
YouTube icon

Using Ultracold Atoms to Model Nuclei and Neutron Matter

September 19, 2011 - 12:30pm
Speaker: 
Ken O'Hara
Institution: 
Penn State

It may seem surprising that a dilute, ultracold atomic gas could share anything in common with nuclei or neutron star matter since the details of their interactions and their absolute energy scales differ so dramatically. Yet when the deBroglie wavelength greatly exceeds the range of interactions and the scattering length is large, universal predictions can be made that apply equally well to both systems. For example, we have observed the Efimov effect, first predicted in the context of nuclear physics, wherein three particles form an infinite geometric sequence of three-body bound states. Our experiments have confirmed this remarkable 40-year-old prediction by observing successive states in the Efimov spectrum of three fermionic lithium atoms and showing that the successive states are related by a universal scale factor. I will also discuss measurements of the universal interaction energy for a strongly-interacting Fermi gas with zero-range interactions that would be relevant to the equation of state for neutron matter at extremely low densities. By recently demonstrating a Fermi system with a large effective range (in addition to a large scattering length), we hope to extend the pertinence of such measurements to neutron matter at densities of astrophysical interest.

1201 Physics Building
College Park, MD 20742

Subscribe to A Quantum Bit 

Quantum physics began with revolutionary discoveries in the early twentieth century and continues to be central in today’s physics research. Learn about quantum physics, bit by bit. From definitions to the latest research, this is your portal. Subscribe to receive regular emails from the quantum world. Previous Issues...

Sign Up Now

Sign up to receive A Quantum Bit in your email!

 Have an idea for A Quantum Bit? Submit your suggestions to jqi-comm@umd.edu