A Southwestern astronomy professor is participating in a project that could add to our knowledge about the early history of the universe.
The project involves the study of intergalactic mediumclouds of gas that are located between the galaxies in the universe. Because these clouds contain primordial material from the beginning of the universe, studying them can provide important clues about the early history of the universe, including galaxy formation.
But it is not easy to study the intergalactic medium. Although the clouds may be hundreds of thousandsif not millionsof light years across, they are of such low density that they cannot be observed directly. The only way to see them is to study how light from more distant galaxies is absorbed as it passes through them. The absorption is revealed in the spectrum, or light signature, of the more distant galaxy. By studying spectra, astronomers can deduce information about the physical properties of clouds, such as density, thickness, temperature, composition and motion.
Studying these clouds requires sophisticated computer models of how light interacts with the gas in intergalactic space, says Mark Bottorff, associate professor of physics.
Bottorff is working on a project to develop these sophisticated computer models. The project is funded by the Space Telescope Science Institute (STSI), which is operated for NASA and headquartered at Johns Hopkins University in Baltimore. The institute oversees all programming related to the Hubble Space Telescope.
The principal researcher on the project is Gary Ferland at the University of Kentucky, who is one of the nations most respected astrophysicists. Bottorff did postdoctoral research with Ferland after completing his Ph.D. in physics at the University of Kentucky.
Ferland developed a computer program known as Cloudy that models the behavior of radiation passing through clouds of gas in space. The code for Cloudy is more than a quarter of a million lines long. Astronomers around the world use Cloudy to do their research. In addition to helping with the study of intergalactic medium, Bottorff notes that Cloudy is also used in other areas of astronomy such as the study of nebulas and quasars.
Bottorff, who has been building computer models for more than 20 years, has a $14,500 grant from STSI to create models that will help validate the Cloudy code. This will give astronomers more confidence that the code is in working order, he says.
His work will model how the clouds are exposed to radiation from the Big Bang (the birth of the universe), as well as more nearby galaxies and energetic quasars. Until now, he explains, models of the clouds have been very simple because computers havent been fast enough to calculate more realistic models.
With every simplification, you are less certain that the model is an accurate description of reality, Bottorff says. Now computers are fast enough that more sophisticated models can be built to carry out these calculations. For example, he says, models can now be created in 2-D and 3-D instead of just 1-D.
This is a great thing for Southwestern because it allows us to be doing astronomy on the cutting edge of astrophysics, Bottorff says.
Kevin ONeil, a junior majoring in physics and business, has been helping Bottorff with his research. ONeil, who plans to pursue graduate studies in either physics or mechanical engineering, says he has thoroughly enjoyed his work on the project.
This experience highlights the benefits provided to students who attend small schools with dedicated and engaging faculty, ONeil says. Dr. Bottorff has provided me with an outstanding learning opportunity.
A Southwestern biology professor received international attention this spring for research he conducted along with two of his former students.
Max Taub, associate professor of biology, Brian Miller 07 and Holly Allen 06, did a meta-analysis of previous research that had been done on the effect of increased atmospheric carbon dioxide on the protein concentrations in barley, rice, wheat, soybean and potato.
Their study found that the crops had significantly lower protein concentrations when grown in atmospheres containing elevated levels of carbon dioxide. Potatoes showed a nearly 14 percent decrease in protein, while the grain crops of barley, rice and wheat showed reductions of 15.3 percent, 9.9 percent and 9.8 percent respectively. The protein decrease in soybeans was much lower, at 1.4 percent.
This is just one more example of the impact global changes could have on us, Taub says. He notes that the impact will be felt the most in poorer countries, where people rely more on plant products for protein.
Taub estimates that 40 percent of human dietary protein worldwide comes from these so-called C3 grains and root crops, both of which show decreased protein concentration at higher levels of atmospheric carbon dioxide.
The study grew out of a question posed by Allen in one of Taubs Global Change Biology classes. For the study, Allen and Miller helped Taub analyze more than 200 experiments that had been previously conducted by other researchers. Their research was published in the March issue of Global Change Biology.
After the study was published online, Taub received numerous requests for interviews from reporters around the world.
Taub is currently studying the impact of increased CO2 concentrations on the mineral composition of foods. Elements such as magnesium, potassium, calcium, iron and zinc are also important for a healthy diet.