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This double-star
system, located approximately 28,000 light-years away in the
constellation Sagittarius, is a source of powerful bursts of
X-ray emission. Argonne physicists have made precise measurements
of exotic isotopes that explain the characteristic X-ray spectrum
and luminosities of such “X-ray bursters.” |
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At the heart of ATLAS—the Argonne Tandem Linac Accelerator System—are these superconducting split-ring resonators, developed at Argonne. ATLAS is the world's first superconducting accelerator for projectiles heavier than the electron, and can be used to accelerate a beam of any atomic nucleus. |
Most precise nuclear mass measurements provide clues to astronomical X-ray bursts |
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Argonne physicists have precisely measured the masses of nuclear isotopes that exist for only fractions of a second or can only be produced in such tiny amounts as to be almost nonexistent in the laboratory. Some isotopes had their masses accurately measured for the first time. The results help explain the characteristic X-ray spectrum and luminosities of strange astronomical objects called “X-ray bursters.” X-ray bursters comprise a normal star and a neutron star. Neutron stars are as massive as our sun but collapsed to 10 miles across. The neutron star’s ferocious gravitational field pulls gas from its companion until the neutron star’s surface ignites in a runaway fusion reaction. For a few tens of seconds, the light from the explosion may be the most brilliant source of X-rays in the sky. The rapid proton-capture process, or “rp-process,” is the dominant source of energy in a common type of X-ray bursters. In this nuclear fusion reaction, nuclei capture protons and transmute into a heavier element, releasing energy in the process. For example, arsenic-67 can capture a proton to become selenium-68. The rp-process proceeds in fits and starts, due to what physicists call “waiting-point nuclei.” Some nuclides, such as selenium-68, can’t absorb an incoming proton as quickly as others can. The reaction must “wait” for the nucleus to absorb a proton—which may take up to 30 minutes, a relative eternity—or for the neutron to decay to a proton, called beta decay, to convert the nuclide into one with a more favorable capture rate. A beta-decay, for example, converts the selenium-68 nucleus into arsenic-68. Arsenic-68 readily captures a proton, changing to selenium-69, and so on. “How long the nova or X-ray burst lasts, and how far the rp-process reactions proceed, is determined by the properties of these few waiting-point nuclei,” said physicist Guy Savard, principal investigator. “Although there are hundreds of nuclei in an X-ray burst, the properties of half a dozen of them make all the difference.” Accurate measurements of waiting-point nuclei masses explain the astronomical observations of X-ray bursts and confirm theories of how they are produced. But measuring their masses is difficult. Some decay in fractions of a second; others can only be produced in such small amounts that standard spectrometry techniques give imprecise results. Argonne’s
Unique ATLAS The created ions are slowed to a crawl in a “gas catcher”—a tube filled with pressurized helium. A gentle electric gradient pulls ions into a Canadian Penning Trap Spectrometer developed by Savard and other scientists at Argonne, the University of Manitoba and McGill University, Montreal, Texas A&M University and the State University of New York. The Penning Trap uses magnetic and electric fields to confine ions. A measurement may involve perhaps only a dozen individual ions, which can stay suspended in the trap for many seconds. Their masses can then be measured using radio-frequency (RF) fields. “The ions will accept energy from the RF field only at certain frequencies,” Savard said. “These frequencies are related to properties of the ion, particularly the mass. By looking at what energies they accept, you can precisely determine the mass.” Ions with previously unknown masses included antimony-107 and -108. The mass of selenium-68 was determined with 30 times more precision than previous, and contradictory, measurements. “This is a unique system, because with the new gas catcher, we can inject any species that can be produced here at ATLAS,” Savard said. “Research is ongoing. We’re now exploring around the tin region, where the rp-process is expected to terminate.” Side bar: Mass measurement experiments are crucial to new accelerator development For more information, please contact David Jacqué. |