Research

Posts related to the research mission of the Physics Department

Faculty Profile: UConn Astrophysicist Cara Battersby

Meet the Researcher: UConn Astrophysicist Cara Battersby

UConn astrophysicist, Cara Battersby. (Carson Stifel/UConn Photo)

A young Cara Battersby once scrawled out the phrase “Science is curious” in a school project about what she wanted to do when she grew up.

This simple phrase still captures Battersby’s outlook on her research about our universe.

Recently shortlisted for the 2018 Nature Research Inspiring Science Award, Battersby has been working on several projects aimed at unfolding some of the most compelling mysteries of galaxies near and far.

“I’m really interested in how stars are born,” Battersby says. “They’re the source of all life on Earth.”

Many of the “laws” we know about how stars are formed are based exclusively on observations of our own galaxy. Because we don’t have as much information about how stars form in other galaxies with different conditions, these laws likely don’t apply as well as we think they should.

Battersby is leading an international team of over 20 scientists to map the center of the Milky Way Galaxy using the Submillimeter Array in Hawaii, in a large survey called CMZoom. She was recently awarded a National Science Foundation grant to follow-up on this survey and create a 3D computer modeled map of the center of the Milky Way Galaxy.

The center of our galaxy has extreme conditions similar to those in other far-off galaxies that are less easily studied, so the Milky Way is an important laboratory for understanding the physics of star formation in extreme conditions.

By mapping out this region in our own galactic backyard, Battersby will be able to form a better idea of how stars form in more remote areas of the universe.

“I love that astrophysics is one of the fields where I can get my hands into everything,” Battersby says. “Stars are something real that you can actually see and study the physics of.”

Battersby is also investigating the “bones” of the Milky Way. Working with researchers from Harvard University, she is looking at how some unusually long clouds could be clues to constructing a more accurate picture of our galaxy.

“Because of the size of our galaxy, it’s infeasible to send a satellite up there to take a picture,” she says.

Since we are living within the Milky Way it is much harder for us to get a clear idea of what it looks like. We know that the Milky Way is a spiral galaxy, but we don’t yet know how many “arms” the spiral has and if it’s even a well-defined spiral.

These kinds of celestial mysteries have long fascinated Battersby.

Battersby says she would “devour” astronomy books and magazines her parents gave her, but it wasn’t until college that her passion truly developed.

She did her Ph.D. thesis at the University of Colorado on high-mass stars being formed on the disk of our galaxy. During this research she made an astounding discovery that every high-density cloud in space is already in some phase of forming a star, a process that takes millions of years.

This led her to conclude that star formation starts as the cloud is collapsing bit by bit, modifying previous ideas of the timeline of this process.

“If you look at something new in a way no one’s looked at it before, the universe has a great way of surprising us,” Battersby says.

View full story on UConn Today.

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By: Anna Zarra Aldrich ’20 (CLAS), Office of the Vice President for Research

 

 

UConn Physics major wins national recognition for research

Connor Occhialini – Finalist 2018 LeRoy Apker Undergraduate Achievements Award

by Jason Hancock

One of our star undergraduates, Connor Occhialini, has won national recognition as a finalist in the 2018 LeRoy Apker Undergraduate Achievements Award competition for his research in the UConn Physics department. The honor and distinction is awarded not only for the excellent research achievements of the student, but also for the department that provides the supportive environment and opportunities for students to excel in research. Connor is in fact the second Apker finalist in three years’ time (Michael Cantara was a 2016 Apker finalist). Connor graduated with a BS in Physics from UConn in May 2018 and stayed on as a researcher during summer 2018. During his time here, he developed theoretical models, helped build a pump-probe laser system, and carried out advanced analysis of X-ray scattering data which revealed a new context for an unusual phenomenon – negative thermal expansion. With these outstanding achievements, the department presented Connor’s nomination to the 2018 LeRoy Apker award committee of the American Physical Society. Connor was selected to be one of only four Apker finalists from all PhD-granting institutions in the US. With this prestigious honor, the department receives a plaque and a $1000 award to support undergraduate research. Connor is now a PhD student in the Physics Department at MIT.

Professor Rainer Weiss: Katzenstein Distinguished Lecture

The Katzenstein Distinguished Lectures series continued in the 2018 academic year with its twenty second Nobel Laureate lecturer, with an October 26, 2018 lecture by Professor Rainer Weiss of the Massachusetts Institute of Technology.

The title of Professor Weiss’ talk was “Exploration of the Universe with Gravitational Waves”, with abstract:

The observations of gravitational waves from the merger of binary black holes and from a binary neutron star coalescence followed by a set of astronomical measurements is an example of investigating the universe by “multi-messenger” astronomy. Gravitational waves will allow us to observe phenomena we already know in new ways as well as to test General Relativity in the limit of strong gravitational interactions – the dynamics of massive bodies traveling at relativistic speeds in a highly curved space-time. Since the gravitational waves are due to accelerating masses while electromagnetic waves are caused by accelerating charges, it is reasonable to expect new classes of sources to be detected by gravitational waves as well. The lecture will start with some basic concepts of gravitational waves, briefly describe the instruments and the methods for data analysis that enable the measurement of gravitational wave strains of one part in 10 to the 21, and then present the results of recent runs. The lecture will end with a vision for the future of gravitational wave astrophysics and astronomy.

Students discuss gravitational waves with Prof. Weiss (MIT) following lecture

In 2017 Professor Weiss shared the Nobel Prize in Physics with Professor Kip Thorne and Professor Barry Barish for their epochal discovery of gravitational waves, waves that had been predicted by Albert Einstein using his General Theory of Relativity no less than a hundred years before.

Professor Rainer Weiss received his BS degree from MIT in 1955 and his PhD from MIT in 1962. He was on the faculty of Tufts University from 1960 to 1962, and did post-doctoral research at Princeton from 1962 to 1964. He joined the MIT faculty in 1964 and remained a regular faculty member there until he became emeritus in 2001. Along with Kip Thorne, the late Ronald Drever and Barry Barish he spearheaded the development of LIGO, the Laser Interferometer Gravitational-Wave Observatory, a set of two interferometers, one located in Louisiana and the other in Washington State. The interferometers would jointly look for gravitational wave signals seen in coincidence, and in September 2015 made the very first detection of gravity waves. At Louisiana State University he has served as an Adjunct Professor of Physics since 2001. As well as research in gravity waves Professor Weiss’ other primary interests are in atomic clocks and cosmic microwave background measurements.

Dr. Weiss had previously visited the University of Connecticut in Fall 2015 as part of a lecture series that fall given at the University of Connecticut in commemoration of the hundredth year of Einstein’s development of his Theory of General Relativity. At that time Dr. Weiss described the ongoing search at LIGO for gravity waves produced by the merger of two black holes. And the initial announcement of a discovery was made in February 2016, shortly after Dr. Weiss’s visit to the University of Connecticut. It is also of interest to note that Dr. Shep Doeleman of Harvard University was another of the speakers at the Fall 2015 University of Connecticut Einstein commemoration. He talked about the ongoing effort to actually detect the event horizons associated with black holes using the Event Horizon Telescope, black holes being yet another prediction of Einstein’s Theory that was also one hundred years old. And in 2019 Dr. Doeleman announced the very the first direct detection of a black hole event horizon. Thus, with the first detection of gravity waves produced by black hole mergers and then the detection of an event horizon itself, the theory of black holes is put on a very secure observational foundation. This lecture can be viewed: https://www.uctv14.com/ucspanblog/2018/12/10/katzenstein-distinguished-lecture-october-26th-2018?rq=Katzenstein

Workshop ‘Dynamic Quantum Matter’ organized by UConn faculty

Dynamic Quantum Matter, Entangled orders and Quantum Criticality Workshop
Dates: June 18- June 19, 2018

Sponsors

UConn, NSF, Nordita, Villum Center for Dirac Materials, Institute for Materials Science – Los Alamos, Wiley Publishers
           

Scope

The conference will focus on entangled and non-equilibrium orders in quantum materials. The 21st century marked the revolution of probing matter at the nano- to mesoscale and these developments continue to be the focus of active research. We now witness equally powerful developments occurring in our understanding, ability to probe, and manipulate quantum matter, in entangled orders and novel states, in the time domain. Recent progress in experimental techniques including x-ray optics, optical pumping, time resolved spectroscopies (ARPES optics), and in cold-atom systems has led to a resurgence of interest in the non-equilibrium aspect of quantum dynamics. The novel entangled orders that have nonzero “overlap” with more than one order parameter also have emerged as an exciting new direction for research in quantum matter. Entangled orders go beyond the conventional orders such as density and spin, and significantly expand the possible condensates we can observe. It is only because of the lack of experimental control, resolution, theoretical framework, and computational power, that the realm of entangled and quantum non-equilibrium remained largely unexplored until now. The time has come for us to turn full attention to these phenomena. Specific topics include: superconductivity and dynamics near quantum criticality, composite orders in correlated materials, effects of strain on quantum critical points, and superconductivity in STO. This conference will have a format of topical lectures, while leaving ample time for discussions.

Venue

Gurney’s Resorts | Newport, RI

Physics undergrad is the recipient of 2018 Mark Miller research award

Physics major Brenna Robertson has been selected as the recipient of the 2018 Mark Miller Undergraduate Research Award. Brenna’s proposal, which focuses on modeling supermassive black hole spin using spectral emission diagrams, was selected from among a strong pool of applicants. Brenna Robertson is working with Prof. Jonathan Trump.

The Mark Miller Award is a stipend to allow a student to remain in Storrs over the Summer session to work on a research project with a faculty member of the Physics Department. It was created through a donation made by Mark E. Miller, a UConn physics major alum.

NASA awards to two physics undergraduate students

Undergraduate Physics Majors, Sam Cutler and Anthony (Josh) Machado, recently received awards from the NASA Connecticut Space Grant Consortium.

Awards recipients Sam Cutler (right) and Josh Machado

Sam was awarded an Undergraduate Research Fellowship to perform research at UConn this summer working with Prof. Kate Whitaker. The title of his research project is “Examining High Redshift Rotation Curve Outside the Local Universe”.

Josh was awarded the Undergraduate Scholarship by the NASA Connecticut Space Grant Consortium, and will be performing astrophysics research this summer at UConn working with Prof. Cara Battersby.

Annual Research Poster Day

The Physics Department Graduate Student Association, in collaboration with the faculty, organized the Annual Research Poster Day which was held this year on March 23, 2018.

Erin Curry presenting her poster “Intermetallic-Superalloy Radiative Heat Transfer in Additive Manufacturing”

About 15 students presented their research in a poster presentation. Awards were presented to graduate students Erin Curry and Martin Disla, and an undergraduate student Sadhana Suresh.

Martin Disla and Prof. Whitaker
Sadhana Suresh and Prof. Niloy Dutta

Prof. Blum has been selected a “Fermilab Distinguished Scholar”

Professor Tom Blum has been selected a “Fermilab Distinguished Scholar”.

Fermilab Distinguished Scholars are rotating multi-year appointments for U.S. theorists in either the Fermilab Theoretical Physics Department or the Theoretical Astrophysics Group.

The Fermilab Distinguished Scholars program aims to:

  • Strengthen connections between the Fermilab Theoretical Physics and Astrophysics groups and the wider U.S. particle-theory community.
  • Broaden the Fermilab theoretical-physics research program through collaborations between the Fermilab Distinguished Scholars and Fermilab theory staff, postdocs, and students.
  • Strengthen connections between the U.S. particle-theory community and the Fermilab experimental program.
  • Increase the frequency and quality of interactions between U.S. particle theorists and Fermilab experimentalists.
  • Increase resident theoretical expertise in targeted physics areas to support the Fermilab experimental program.

For more information see Fermilab Distinguished Scholars Program