Tag: SMU Department of Physics

SMU physicists celebrate Nobel Prize for discovery of Higgs boson “god particle”

Post author By Margaret Allen
Post date October 8, 2013

SMU joins nearly 2,000 physicists from U.S. institutions — including 89 U.S. universities and seven U.S. DOE labs — that participate in discovery experiments

SMU’s experimental physics group played a pivotal role in discovering the Higgs boson — the particle that proves the theory for which two scientists have received the 2013 Nobel Prize in Physics.

The Royal Swedish Academy of Sciences today awarded the Nobel Prize to theorists Peter W. Higgs and François Englert to recognize their work developing the theory of what is now known as the Higgs field, which gives elementary particles mass. U.S. scientists played a significant role in advancing the theory and in discovering the particle that proves the existence of the Higgs field, the Higgs boson.

The Nobel citation recognizes Higgs and Englert “for the theoretical discovery of a mechanism that contributes to our understanding of the origin of mass of subatomic particles, and which recently was confirmed through the discovery of the predicted fundamental particle, by the ATLAS and CMS experiments at CERN’s Large Hadron Collider.”

In the 1960s, Higgs and Englert, along with other theorists, including Robert Brout, Tom Kibble and Americans Carl Hagen and Gerald Guralnik, published papers introducing key concepts in the theory of the Higgs field. In 2012, scientists on the international ATLAS and CMS experiments, performed at the Large Hadron Collider at CERN laboratory in Europe, confirmed this theory when they announced the discovery of the Higgs boson.

“A scientist may test out a thousand different ideas over the course of a career. If you’re fortunate, you get to experiment with one that works,” says SMU physicist Ryszard Stroynowski, a principal investigator in the search for the Higgs boson. As the leader of an SMU Department of Physics team working on the experiment, Stroynowski served as U.S. coordinator for the ATLAS Experiment’s Liquid Argon Calorimeter, which measures energy from the particles created by proton collisions.

The University’s experimental physics group has been involved since 1994 and is a major contributor to the research, the heart of which is the Large Hadron Collider particle accelerator on the border with Switzerland and France.

SMU joins nearly 2,000 physicists from U.S. institutions — including 89 U.S. universities and seven U.S. Department of Energy laboratories — that participate in the ATLAS and CMS experiments, making up about 23 percent of the ATLAS collaboration and 33 percent of CMS at the time of the Higgs discovery. Brookhaven National Laboratory serves as the U.S. hub for the ATLAS experiment, and Fermi National Accelerator Laboratory serves as the U.S. hub for the CMS experiment. U.S. scientists provided a significant portion of the intellectual leadership on Higgs analysis teams for both experiments.

Preliminary discovery results were announced July 4, 2012 at CERN, the European Organization for Nuclear Research, near Geneva, Switzerland, and at the International Conference of High Energy Physics in Melbourne, Australia.

“It is an honor that the Nobel Committee recognizes these theorists for their role in predicting what is one of the biggest discoveries in particle physics in the last few decades,” said Fermilab Director Nigel Lockyer. “I congratulate the whole particle physics community for this achievement.”

The majority of U.S. scientists participating in LHC experiments work primarily from their home institutions, remotely accessing and analyzing data through high-capacity networks and grid computing. The United States plays an important role in this distributed computing system, providing 23 percent of the computing power for ATLAS and 40 percent for CMS. The United States also supplied or played a leading role in several main components of the two detectors and the LHC accelerator, amounting to a value of $164 million for the ATLAS detector, $167 million for the CMS detector, and $200 million for the LHC. Support for the U.S. effort comes from the U.S. Department of Energy Office of Science and the National Science Foundation.

“It’s wonderful to see a 50-year-old theory confirmed after decades of hard work and remarkable ingenuity,” said Brookhaven National Laboratory Director Doon Gibbs. “The U.S. has played a key role, contributing scientific and technical expertise along with essential computing and data analysis capabilities — all of which were necessary to bring the Higgs out of hiding. It’s a privilege to share in the success of an experiment that has changed the face of science.”

The discovery of the Higgs boson at CERN was the culmination of decades of effort by physicists and engineers around the world, at the LHC but also at other accelerators such as the Tevatron accelerator, located at Fermilab, and the Large Electron Positron accelerator, which once inhabited the tunnel where the LHC resides. Work by scientists at the Tevatron and LEP developed search techniques and eliminated a significant fraction of the space in which the Higgs boson could hide.

Several contributors from SMU have made their mark on the project at various stages, including current Department of Physics faculty members Ryszard Stroynowski, Jingbo Ye, Robert Kehoe and Stephen Sekula. Faculty members Pavel Nadolsky and Fred Olness performed theoretical calculations used in various aspects of data analysis.

University postdoctoral fellows on the ATLAS Experiment have included Julia Hoffmann, David Joffe, Ana Firan, Haleh Hadavand, Peter Renkel, Aidan Randle-Conde and Daniel Goldin.

SMU has awarded eight Ph.D. and seven M.Sc. degrees to students who performed advanced work on ATLAS, including Ryan Rios, Rozmin Daya, Renat Ishmukhametov, Tingting Cao, Kamile Dindar, Pavel Zarzhitsky and Azzedin Kasmi.

Significant contributions to ATLAS have also been made by SMU faculty members in the Department of Physics’ Optoelectronics Lab, including Tiankuan Liu, Annie Xiang and Datao Gong.

“The discovery of the Higgs is a great achievement, confirming an idea that will require rewriting of the textbooks,” Stroynowski says. “But there is much more to be learned from the LHC and from ATLAS data in the next few years. We look forward to continuing this work.”

Higgs and Englert published their papers independently and did not meet in person until the July 4, 2012, announcement of the discovery of the Higgs boson at CERN. Higgs, 84, is a professor emeritus at the University of Edinburgh in Scotland. Englert, 80, is a professor emeritus at Universite Libre de Bruxelles in Belgium.

The prize was announced at 5:45 a.m. CDT on Tuesday, Oct. 8, 2013.

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SMU is a nationally ranked private university in Dallas founded 100 years ago. Today, SMU enrolls nearly 11,000 students who benefit from the academic opportunities and international reach of seven degree-granting schools. For more information see www.smu.edu.

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Tags Annie C. Xiang, Dedman College, Fredrick Olness, Jingbo Ye, Julia Hoffman, Pavel Nadolsky, Robert Kehoe, Ryan Rios, Ryszard Stroynowski, SMU Department of Physics, Stephen J. Sekula

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NOvA neutrino detector in Minnesota records first 3-D particle tracks in search to understand universe

Post author By Margaret Allen
Post date March 28, 2013

The NOvA detector, currently under construction in Ash River, Minn., stands about 50 feet tall and 50 feet wide. The completed detector will weigh 14,000 tons. (Credit: Fermilab)

What will soon be the most powerful neutrino detector in the United States has recorded its first three-dimensional images of particles.

Using the first completed section of the NOvA neutrino detector under construction in Minnesota, scientists have begun collecting data from cosmic rays—particles produced by a constant rain of atomic nuclei falling on the Earth’s atmosphere from space.

Scientists’ goal for the completed detector is to use it to discover properties of mysterious fundamental particles called neutrinos.

Neutrinos are as abundant as cosmic rays in the atmosphere, but they have barely any mass and interact much more rarely with other matter. Many of the neutrinos around today are thought to have originated in the Big Bang when the universe began.

“These recent tests with the very first portions of our eventual 14,000-ton detector are extremely gratifying since they give us confidence that after many years of work by many people, and innumerable design meetings, our detector is actually becoming alive,” said physicist Thomas E. Coan, an associate professor of physics at Southern Methodist University. “There now seem to be no fundamental show stoppers lurking around.”

SMU hosted in January the most recent general meeting for the experiment known by the acronym NOvA.

“That was the last meeting before these tests were completed and it allowed us to settle details of the tests and make sure they would be crisp and meaningful,” Coan said. “Overall, understanding neutrinos is essential to understanding our universe at a deep level. But studying them is also considerable fun since they are so weird.”

The active section of the detector, under construction in Ash River, Minn., is about 12 feet long, 15 feet wide and 20 feet tall. The full detector will measure more than 200 feet long, 50 feet wide and 50 feet tall.

“It’s taken years of hard work and close collaboration among universities, national laboratories and private companies to get to this point,” said Pier Oddone, director of the Department of Energy’s Fermi National Accelerator Laboratory. Fermilab manages the project to construct the detector.

“The more we know about neutrinos, the more we know about the early universe and about how our world works at its most basic level,” said NOvA co-spokesperson Gary Feldman of Harvard University.

“A possible path to understanding why any matter at all is present in our universe — including the matter that comprises us — is to understand the behavior of neutrinos, which are especially mysterious subatomic particles,” said SMU’s Coan.

“Neutrinos are almost a billion times more numerous in the universe than hydrogen, the universe’s most abundant element. But with a mass more than a million times smaller than an electron’s, the electrically neutral neutrino interacts extraordinarily feebly with matter,” he said. “A common reference scale is that a neutrino needs to travel a distance of a light year through lead before it will interact with another particle. Neutrinos also have the peculiar property that they morph from one type — or “flavor” — to another as they travel.”

Later this year, Fermilab, outside of Chicago, will start sending a beam of neutrinos 500 miles through the earth to the NOvA detector near the Canadian border. When a neutrino interacts in the NOvA detector, the particles it produces leave trails of light in their wake. The detector records these streams of light, enabling physicists to identify the original neutrino and measure the amount of energy it had.

“The morphing of a muon flavor neutrino to an electron flavor neutrino is particularly interesting,” Coan said, noting that the flavor of a neutrino is determined by what electrically charged particles it produces when it eventually interacts with matter. “An electron neutrino produces electrons while a muon neutrino produces a muon, which is a kind of heavy, radioactive electron.”

The whole phenomenon of neutrino morphing — called “neutrino flavor oscillation” — is poorly understood, he said, but needs to be if neutrino interactions in the early universe can be sensibly thought to be central to explaining the subsequent absence of antimatter.

“NOνA will produce large numbers of muon neutrinos in the particle beam. The far detector contains enough target nuclei for the neutrinos to interact with,” Coan said. “The far distance between source and detector allows time for the muon neutrinos to morph into electron neutrinos. NOνA will detect the morphing of muon neutrinos into electron neutrinos by detecting the creation of electrons in the far detector. Measuring the frequency of this particular morphing is one important science goal.”

When cosmic rays pass through the NOvA detector, they leave straight tracks and deposit well-known amounts of energy. They are great for calibration, said Mat Muether, a Fermilab post-doctoral researcher who has been working on the detector.

“Everybody loves cosmic rays for this reason,” Muether said. “They are simple and abundant and a perfect tool for tuning up a new detector.”

The detector at its current size catches more than 1,000 cosmic rays per second. Naturally occurring neutrinos from cosmic rays, supernovae and the sun stream through the detector at the same time. But the flood of more visible cosmic ray data makes it difficult to pick them out.

Once the upgraded Fermilab neutrino beam starts later this year, the NOvA detector will take data every 1.3 seconds to synchronize with the Fermilab accelerator. Inside this short time window, the burst of neutrinos from Fermilab will be much easier to spot.

The NOvA detector will be operated by the University of Minnesota under a cooperative agreement with the U.S. Department of Energy’s Office of Science.

The NOvA experiment is a collaboration of 180 scientists, technicians and students from 20 universities and laboratories in the U.S and another 14 institutions around the world. The scientists are funded by the U.S. Department of Energy, the National Science Foundation and funding agencies in the Czech Republic, Greece, India, Russia and the United Kingdom.

Follow SMUResearch.com on Twitter.

For more information, www.smuresearch.com.

SMU is a nationally ranked private university in Dallas founded 100 years ago. Today, SMU enrolls nearly 11,000 students who benefit from the academic opportunities and international reach of seven degree-granting schools. For more information see www.smu.edu.

Tags Dedman College, SMU Department of Physics, Thomas E. Coan

Earth & Climate Energy & Matter Researcher news SMU In The News Student researchers

UPI: Cosmic explosions give dark energy clues

Post author By Margaret Allen
Post date March 4, 2013

The international news wire service United Press International has covered the SMU Physics Department’s recent supernovae discoveries. The article, “Cosmic explosions give dark energy clues,” was published Feb. 27. Light from two massive stars that exploded hundreds of millions of years ago recently reached Earth, and each event was identified as a supernova by SMU graduate students in the physics department.

Both supernovae were spotted with the Robotic Optical Transient Search Experiment‘s robotic telescope ROTSE3b, which is now operated by SMU graduate students. ROTSE3b is at the McDonald Observatory in the Davis Mountains of West Texas near Fort Davis.

The Central Bureau for Astronomical Telegrams of the International Astronomical Union officially designated the discoveries as Supernova 2013X and Supernova 2012ha.

Ferrante and Dhungana made both discoveries as part of an international collaboration of physicists from nine universities. Everest and Sherpa were discovered with a fully automated, remotely controlled robotic telescope at the University of Texas’ McDonald Observatory. The discovery is a first for the SMU collaboration members.

See the article.

EXCERPT:

DALLAS, Feb. 27 (UPI) — Light from exploding stars is improving the astronomical “yardstick” used to calculate the acceleration of the expansion of the universe, U.S. scientists say.

The light from two supernovae, massive stars that exploded hundreds of millions of years ago, has recently reached Earth, Southern Methodist University researchers said.

A supernova discovered Feb. 6 exploded about 450 million years ago, while a second supernova discovered Nov. 20 exploded about 230 million years ago, Farley Ferrante, an SMU graduate student who made the initial Feb. 6 observation, said.

Both are Type 1a supernovae, the result of white dwarf explosions, he said.

“We call these Type 1a supernovae standard candles,” Ferrante said. “Since Type 1a supernovae begin from this standard process, their intrinsic brightness is very similar. So they become a device by which scientists can measure cosmic distance.”

Type 1a supernova provide astronomers with indirect information about dark energy, which makes up 73 percent of the mass-energy in the universe and is theorized as being responsible for the accelerating expansion of our universe at various times after the Big Bang.

“Every exploding star observed allows astronomers to more precisely calibrate the increasing speed at which our universe is expanding,” Ferrante said. “The older the explosion, the farther away, the closer it was to the Big Bang and the better it helps us understand dark energy.”

See the article.

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Tags Dedman College, Farley Ferrante, Govinda Dhungana, Robert Kehoe, SMU Department of Physics

Earth & Climate Energy & Matter Researcher news SMU In The News Student researchers

ANI News: Exploding stars offer clues to dark energy

Post author By Margaret Allen
Post date March 4, 2013

The Asian news wire service Asian News International has covered the SMU Physics Department’s recent supernovae discoveries. The article, “Exploding stars offer clues to dark energy,” was published Feb. 28. Light from two massive stars that exploded hundreds of millions of years ago recently reached Earth, and each event was identified as a supernova by SMU graduate students in the physics department.

The Central Bureau for Astronomical Telegrams of the International Astronomical Union officially designated the discoveries as Supernova 2013X and Supernova 2012ha.

Read the full article.

EXCERPT:

Washington, February 28 (ANI): Observation of two bright exploding stars is improving the astronomical “tape measure” used to calculate the acceleration of the expansion of the universe, say scientists.

Light from two massive stars that exploded hundreds of millions of years ago recently reached Earth, and each event was identified as a supernova, Southern Methodist University scientists said.

A supernova discovered Feb. 6 exploded about 450 million years ago, said Farley Ferrante, a graduate student at Southern Methodist University, Dallas, who made the initial observation.

The exploding star is in a relatively empty portion of the sky labeled “anonymous” in the faint constellation Canes Venatici. Home to a handful of galaxies, Canes Venatici is near the constellation Ursa Major , best known for the Big Dipper.

A second supernova discovered Nov. 20 exploded about 230 million years ago, said Ferrante, who made the initial observation. That exploding star is in one of the many galaxies of the Virgo constellation.

Both supernovae were spotted with the Robotic Optical Transient Search Experiment’s robotic telescope ROTSE3b, which is now operated by SMU graduate students. ROTSE3b is at the McDonald Observatory in the Davis Mountains of West Texas near Fort Davis.

The supernova that exploded about 450 million years ago is officially designated Supernova 2013X. It occurred when life on Earth consisted of creatures in the seas and oceans and along coastlines. Following naming conventions for supernova, Supernova 2013X was nicknamed “Everest” by Govinda Dhungana, an SMU graduate student who participated in the discovery.

The supernova that exploded about 230 million years ago is officially designated Supernova 2012ha. The light from that explosion has been en route to Earth since the Triassic geologic period, when dinosaurs roamed the planet.

“That’s fairly recent as these explosions go,” Ferrante said.

Dhungana gave the nickname “Sherpa” to Supernova 2012ha.

Everest and Sherpa are two of about 200 supernovae discovered worldwide in a given year, according to the scientists.

“Everest and Sherpa aren’t noteworthy for being the youngest, oldest, closest, furthest or biggest supernovae ever observed. But both, like other supernovae of their kind, are important because they provide us with information for further science,” Ferrante said.

Read the full article.

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Tags Dedman College, Farley Ferrante, Govinda Dhungana, Robert Kehoe, SMU Department of Physics

Earth & Climate Energy & Matter Researcher news SMU In The News Student researchers

redOrbit: Astronomers Discover White Dwarf Supernovae

Post author By Margaret Allen
Post date March 1, 2013

The news web site redOrbit has covered the SMU Physics Department’s recent supernovae discoveries. The article, “Astronomers Discover White Dwarf Supernovae,” was published Feb. 27. Light from two massive stars that exploded hundreds of millions of years ago recently reached Earth, and each event was identified as a supernova by SMU graduate students in the physics department.

The Central Bureau for Astronomical Telegrams of the International Astronomical Union officially designated the discoveries as Supernova 2013X and Supernova 2012ha.

Read the full article.

EXCERPT:

By Lee Rannals
redOrbit.com
White dwarf supernovae that occurred millions of years ago have popped up in the Virgo Cluster galaxy and part of the sky labelled as “anonymous.”

Southern Methodist University (SMU) researchers say they’ve confirmed two bright stars that showed up in our skies in February and November are supernovae. Supernovae are the result of stars that have reached the end of their life, resulting in a large explosion that can consume anything in its path.

In November, Farley Ferrante, a graduate student at SMU, made the initial observation of a supernova, Supernova 2012ha or “Sherpa,” that derived from the Virgo constellation, about 230 million light years away. Another supernova, Supernova 2013X or “Everest,” was discovered on February 6, sitting 450 million years away in a part of the sky labeled “animus” near the faint constellation Canes Venatici.

“Everest and Sherpa aren’t noteworthy for being the youngest, oldest, closest, furthest or biggest supernovae ever observed,” Ferrante said. “But both, like other supernovae of their kind, are important because they provide us with information for further science.”

Both supernovae are considered Type 1a, which are the result of white dwarf explosions. A white dwarf star has a mass comparable to that of the Sun and its core is a comparable size to that of the Earth. According to Robert Kehoe, physics professor and leader of the SMU astronomy team in the SMU Department of Physics, a teaspoon of a white dwarf star would weigh about as much as Mount Everest.

When a white dwarf heads towards the end of its life, it grows to about one and a half times the size of the sun and eventually collapses and explodes, resulting in a Type 1a supernova.

“We call these Type 1a supernovae standard candles,” Ferrante said. “Since Type 1a supernovae begin from this standard process, their intrinsic brightness is very similar. So they become a device by which scientists can measure cosmic distance. From Earth, we measure the light intensity of the exploded star. As star distances from Earth increase, their brilliance diminishes.”

Read the full article.

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Tags Dedman College, Farley Ferrante, Govinda Dhungana, Robert Kehoe, SMU Department of Physics

SMU joins nearly 2,000 physicists from U.S. institutions — including 89 U.S. universities and seven U.S. DOE labs — that participate in discovery experiments

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