Artemis Spyrou

Last updated
Artemis Spyrou
Artemisia Spyrou
Artemis Spyrou experimental nuclear astrophysicist.jpg
NationalityCyprus
Education National (Metsovian) Technical University of Athens
Awards National Science Foundation CAREER Awards
Scientific career
Fields Nuclear astrophysics, Nuclear Physics
Institutions Michigan State University, National Superconducting Cyclotron Laboratory
Website https://www.nscl.msu.edu/directory/spyrou.html

Artemisia (Artemis) Spyrou is an experimental nuclear astrophysicist and professor at Michigan State University. She is also the Associate Director for Education and Outreach [1] at the National Superconducting Cyclotron Laboratory. She was the recipient of a NSF CAREER Award. [2]

Contents

Early life and education

Spyrou was born in Limassol, Cyprus. She received an undergraduate degree in physics from the Aristotle University of Thessaloniki in 2001 and a master's degree in physics from the National Technical University of Athens in 2003. [3] She received a PhD from the Institute of Nuclear Physics of the National Centre of Scientific Research "Demokritos" and National Technical University of Athens in 2007, where she studied experimental nuclear astrophysics using the Dynamitron Tandem accelerator (DTL) at the University of Bochum. [3]

Research

Spyrou is an experimental physicist who uses the isotope beams at the National Superconducting Cyclotron Laboratory to study how the elements are made in the universe. [4] With particular regard to the r-process and s-process of neutron capture. By analyzing the resulting beta-decay from neutron capture reactions using the SuN Detector [5] with techniques developed by her group.

Recognition

In 2011, Spyrou was awarded the Thomas H. Osgood Faculty Teaching Award [6] from the department of Physics and Astronomy at Michigan State University for her dedication to undergraduate education in the department. She was also featured on an episode of PBS Curious Crew. [7]

In 2021, she was named a Fellow of the American Physical Society (APS), after a nomination from the APS Division of Nuclear Physics, "for studies using total absorption spectroscopy and the beta-Oslo technique to determine neutron-capture rates for astrophysical modeling, and for dedication to communicating science to the general public". [8]

Selected works

Related Research Articles

Neutronium is a hypothetical substance made purely of neutrons. The word was coined by scientist Andreas von Antropoff in 1926 for the hypothetical "element of atomic number zero" that he placed at the head of the periodic table. However, the meaning of the term has changed over time, and from the last half of the 20th century onward it has been also used to refer to extremely dense substances resembling the neutron-degenerate matter theorized to exist in the cores of neutron stars; hereinafter "degenerate neutronium" will refer to this.

<span class="mw-page-title-main">Island of stability</span> Predicted set of isotopes of relatively more stable superheavy elements

In nuclear physics, the island of stability is a predicted set of isotopes of superheavy elements that may have considerably longer half-lives than known isotopes of these elements. It is predicted to appear as an "island" in the chart of nuclides, separated from known stable and long-lived primordial radionuclides. Its theoretical existence is attributed to stabilizing effects of predicted "magic numbers" of protons and neutrons in the superheavy mass region.

<span class="mw-page-title-main">Neutron flux</span> Total distance traveled by neutrons within a volume over a time period

The neutron flux is a scalar quantity used in nuclear physics and nuclear reactor physics. It is the total distance travelled by all free neutrons per unit time and volume. Equivalently, it can be defined as the number of neutrons travelling through a small sphere of radius in a time interval, divided by a maximal cross section of the sphere and by the duration of the time interval. The dimension of neutron flux is and the usual unit is cm−2s−1.

<span class="mw-page-title-main">Isotopes of hydrogen</span> Hydrogen with different numbers of neutrons

Hydrogen (1H) has three naturally occurring isotopes, sometimes denoted 1
H
, 2
H
, and 3
H
. 1
H
and 2
H
are stable, while 3
H
has a half-life of 12.32(2) years. Heavier isotopes also exist, all of which are synthetic and have a half-life of less than one zeptosecond (10−21 s). Of these, 5
H
is the least stable, while 7
H
is the most.

Thorium (90Th) has seven naturally occurring isotopes but none are stable. One isotope, 232Th, is relatively stable, with a half-life of 1.405×1010 years, considerably longer than the age of the Earth, and even slightly longer than the generally accepted age of the universe. This isotope makes up nearly all natural thorium, so thorium was considered to be mononuclidic. However, in 2013, IUPAC reclassified thorium as binuclidic, due to large amounts of 230Th in deep seawater. Thorium has a characteristic terrestrial isotopic composition and thus a standard atomic weight can be given.

Naturally occurring xenon (54Xe) consists of seven stable isotopes and two very long-lived isotopes. Double electron capture has been observed in 124Xe and double beta decay in 136Xe, which are among the longest measured half-lives of all nuclides. The isotopes 126Xe and 134Xe are also predicted to undergo double beta decay, but this process has never been observed in these isotopes, so they are considered to be stable. Beyond these stable forms, 32 artificial unstable isotopes and various isomers have been studied, the longest-lived of which is 127Xe with a half-life of 36.345 days. All other isotopes have half-lives less than 12 days, most less than 20 hours. The shortest-lived isotope, 108Xe, has a half-life of 58 μs, and is the heaviest known nuclide with equal numbers of protons and neutrons. Of known isomers, the longest-lived is 131mXe with a half-life of 11.934 days. 129Xe is produced by beta decay of 129I ; 131mXe, 133Xe, 133mXe, and 135Xe are some of the fission products of both 235U and 239Pu, so are used as indicators of nuclear explosions.

Calcium (20Ca) has 26 known isotopes, ranging from 35Ca to 60Ca. There are five stable isotopes, plus one isotope (48Ca) with such a long half-life that it is for all practical purposes stable. The most abundant isotope, 40Ca, as well as the rare 46Ca, are theoretically unstable on energetic grounds, but their decay has not been observed. Calcium also has a cosmogenic isotope, 41Ca, with half-life 99,400 years. Unlike cosmogenic isotopes that are produced in the air, 41Ca is produced by neutron activation of 40Ca. Most of its production is in the upper metre of the soil column, where the cosmogenic neutron flux is still strong enough. 41Ca has received much attention in stellar studies because it decays to 41K, a critical indicator of solar system anomalies. The most stable artificial isotopes are 45Ca with half-life 163 days and 47Ca with half-life 4.5 days. All other calcium isotopes have half-lives of minutes or less.

Roentgenium (111Rg) is a synthetic element, and thus a standard atomic weight cannot be given. Like all synthetic elements, it has no stable isotopes. The first isotope to be synthesized was 272Rg in 1994, which is also the only directly synthesized isotope; all others are decay products of heavier elements. There are seven known radioisotopes, having mass numbers of 272, 274, and 278–282. The longest-lived isotope is 282Rg with a half-life of about 2 minutes, although the unconfirmed 283Rg and 286Rg may have longer half-lives of about 5.1 minutes and 10.7 minutes respectively.

Bismuth-209 (209Bi) is an isotope of bismuth, with the longest known half-life of any radioisotope that undergoes α-decay. It has 83 protons and a magic number of 126 neutrons, and an atomic mass of 208.9803987 amu. Primordial bismuth consists entirely of this isotope.

<span class="mw-page-title-main">Daya Bay Reactor Neutrino Experiment</span> Particle physics experiment studying neutrinos

The Daya Bay Reactor Neutrino Experiment is a China-based multinational particle physics project studying neutrinos, in particular neutrino oscillations. The multinational collaboration includes researchers from China, Chile, the United States, Taiwan, Russia, and the Czech Republic. The US side of the project is funded by the US Department of Energy's Office of High Energy Physics.

G. Norris Glasoe was an American nuclear physicist. He was a member of the Columbia University team which was the first in the United States to verify the European discovery of the nuclear fission of uranium via neutron bombardment. During World War II, he worked at the MIT Radiation Laboratory. He was a physicist and administrator at the Brookhaven National Laboratory.

The Modular Neutron Array (MoNA) is a large-area, high-efficiency neutron detector that is used in basic research of rare isotopes at Michigan State University's National Superconducting Cyclotron Laboratory (NSCL), a nuclear physics research facility. It is specifically designed for detecting neutrons stemming from breakup reactions of fast fragmentation beams.

<span class="mw-page-title-main">Kevin Insik Hahn</span> South Korean physicist (born 1962)

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<span class="mw-page-title-main">Michael C. F. Wiescher</span>

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<span class="mw-page-title-main">ISOLDE Decay Station experiment</span>

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References

  1. "Organization of the NSCL Laboratory". Organization of the NSCL Laboratory. Retrieved 24 October 2019.
  2. "NSF Award Search: Award#1350234 - CAREER:beta-decay experiments to constrain astrophysical processes". www.nsf.gov. Retrieved 2019-10-24.
  3. 1 2 "Home". artemisspyrou. Retrieved 2019-10-25.
  4. Thomas, Jessica (February 28, 2019). "Q&A: Studying the Stars—No Telescope Required". Physics. 12: 22. Bibcode:2019PhyOJ..12...22.. doi:10.1103/Physics.12.22. Archived from the original on 2019-02-28. Retrieved October 24, 2019.
  5. "SuN Detector". SuN Detector.
  6. "Thomas H. Osgood Faculty Teaching Awards".
  7. "Curious Crew on PBS". PBS Curious Crew. Retrieved 24 October 2019.
  8. "Fellows nominated in 2021 by the Division of Nuclear Physics". APS Fellows archive. American Physical Society. Retrieved 2021-10-22.