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Cheating to create the perfect simulation: Physicists on way to describing inside of neutron stars

Date:
January 17, 2013
Source:
Friedrich-Schiller-Universitaet Jena
Summary:
Scientists have succeeded in simulating the strong atomic nuclear interactions to enable its calculability while at the same time preserving the typical characteristics of a neutron star.

The planet Earth will die -- if not before, then when the Sun col­lapses. This is going to happen in approximately seven billion years. In the uni­verse however the death of suns and planets is an everyday occurance and our solar system partly consists of their remnants.

The end of stars -- suns -- rich in mass is often a neutron star. These "stars' liches" demonstrate a high density, in which atoms are extremely compressed. Such neutron stars are no bigger than a small town, but hea­vier than our sun, as physicist PD Dr. Axel Maas of the Jena University (Germany) points out. He adds: "The atomic nuclei are very densely packed." Compared to ato­ms, like water, the nuclei of neutron stars are as tightly packed as a bus with 1.000 pas­sengers crowded together in comparison to a bus with only the driver on board. In these densely packed atomic nuclei, so-called "nuclear forces" are at work. They keep the neutron star together and are responsible for its "eternal life" -- and for the last 35 years the strong nuclear interactions were amongst the greatest challenges of theoretical physics.

First Theory for such a Tight Package

Together with colleagues from the Universities of Jena and Darmstadt (both Germany) Axel Maas has succeeded in simulating the strong atomic nuclear interactions to enable its calculability while at the same time preserving the typical charac­teristics of a neutron star. "It is the first theory for such a tight package," the Jena Physicist says. Previously simulations trying to specify the matter inside of neutron stars collapsed far too much in size and yielded the wrong properties time and again -- even on the most powerful computers. "These simulations didn't work because there are too many atomic nuclei," Maas explains the problem, whose solution the world of physics has come closer to due to the calculations of the Jena researchers. To get there, the scientists did so many calculations at the Loewe Center for Science Com­puting (CSC) in Frankfurt, that it would have taken a single PC approximately 2.500 years to do the same.

"We weren't able to solve the initial problem either," Axel Maas concedes, as algorithms are not (yet) powerful enough. However, the Jena physi­cist who had been researching this problem since 2007 and his colleagues "reached a new level of quality." They found a "modification of the theory for such a tight package," Maas says. And thus they enabled nuclear material to be simulated. Most characteristics of the neutron star are being preserved with the Jena method, but now they enabled its cal­culability.

Intelligently Modifyed the Nu­clear Forces

The team accomplished this big step forward by intelligently modifying the nu­clear forces and by solving the stacking problem of the atoms. That they were at the same time 'cheating a bit', the physicists freely admit. However, Maas firmly believes: "We found the best possible shortcut." Now they know "what is relevant for the original simulation."

Now this new verifying method is available for numerous questions and theories about neutron stars and very dense atomic nuclei packages. Maas already knows of first groups of scientists who are planning to use the Jena findings to work with them and to carry them further. The scientists involved are already in the pro­cess of enlarging the simulation and to verify the results: the results enabling scientists to understand the inside of neutron stars eventually.


Story Source:

The above story is based on materials provided by Friedrich-Schiller-Universitaet Jena. Note: Materials may be edited for content and length.


Journal Reference:

  1. Axel Maas, Lorenz von Smekal, Björn Wellegehausen, Andreas Wipf. Phase diagram of a gauge theory with fermionic baryons. Physical Review D, 2012; 86 (11) DOI: 10.1103/PhysRevD.86.111901

Cite This Page:

Friedrich-Schiller-Universitaet Jena. "Cheating to create the perfect simulation: Physicists on way to describing inside of neutron stars." ScienceDaily. ScienceDaily, 17 January 2013. <www.sciencedaily.com/releases/2013/01/130117133215.htm>.
Friedrich-Schiller-Universitaet Jena. (2013, January 17). Cheating to create the perfect simulation: Physicists on way to describing inside of neutron stars. ScienceDaily. Retrieved October 23, 2014 from www.sciencedaily.com/releases/2013/01/130117133215.htm
Friedrich-Schiller-Universitaet Jena. "Cheating to create the perfect simulation: Physicists on way to describing inside of neutron stars." ScienceDaily. www.sciencedaily.com/releases/2013/01/130117133215.htm (accessed October 23, 2014).

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