Physics

Susan is broadly interested in astrophysical magnetism and the physics of the interstellar medium (ISM), from diffuse gas to dense, star-forming regions. Susan’s research tackles open questions like the structure of the Milky Way’s magnetic field, the nature of interstellar turbulence and the multi-phase ISM, and the role of magnetism in star formation. These big questions demand multiwavelength observations and new data analysis techniques. Susan and her group decipher the magnetic ISM using a combination of theory and observation.

The research interests of the molecular imaging instrumentation lab are to create novel instrumentation and software algorithms for in vivo imaging of molecular signatures of disease in humans and small laboratory animals. These new cameras efficiently image radiation emissions in the form of positrons, annihilation photons, gamma rays, and/or light emitted from molecular contrast agents that were introduced into the body and distributed in the subject tissues.

Susan is broadly interested in astrophysical magnetism and the physics of the interstellar medium (ISM), from diffuse gas to dense, star-forming regions. Susan’s research tackles open questions like the structure of the Milky Way’s magnetic field, the nature of interstellar turbulence, and the role of magnetism in star formation. These big questions demand multiwavelength observations and new data analysis techniques.

How did the Universe form and evolve and what is it made of? Our group works on a range of topics in cosmology and astrophysics, with a focus on the formation of cosmological structure in the Universe, its impact on galaxy formation, and its use in determining the nature of dark matter and dark energy.

Together with Dan Akerib, Tom works on the LUX and LZ dark matter experiments to search for dark matter in the form of Weakly Interacting Massive Particles, or WIMPs. The detectors use liquid xenon as a target medium in a time projection chamber, or TPC. The Large Underground Xenon (LUX) experiment is currently operating a 250-kg target in the former Homestake gold mine in the Black Hills of South Dakota. Preparations are underway atSLAC to design and build the 7-ton successor, known as LUX-ZEPLIN (LZ).

Phil's main research interests are in the structure and dynamics of the interior of the sun, how this affect solar activity and through this its effects on terrestrial systems. Phil's group’s primary emphasis is on the structure and dynamics of the solar interior using techniques of helioseismology. His group are interested in both developing instrumentation for solar observatories and in the data analysis of solar magnetic fields from space and from the ground.

Aaron's current research focus is the study of dark energy using images from the ongoing Dark Energy Survey (DES) and the  future Large Synoptic Survey Telescope (LSST). He is interested in studying dark energy using both galaxy clusters and weak gravitational lensing. His research group connects instrumental work, in particular active optics and wavefront measurements at DES and a program of camera-wide testing at LSST,  with cosmology measurements.

Roger is interested in a variety of topics in high energy astrophysics and cosmology. Much of Roger's group are currently focused on understanding the cosmic gamma-ray sources discovered by the Fermi Space telescope, principally pulsars and blazars. This inherently multi-wavelength question requires them to use telescopes all over the world and in space in order to assemble data on these objects and then to develop and test theoretical models to explain what we see.

Our group works with  adaptive optics - optical systems that correct for aberrations using mirrors that change their shape thousands of times per second. This can allow telescopes located on the Earth to correct for atmospheric turbulence and produce diffraction-limited images, which we use to study giant extrasolar planets through direct imaging with the Gemini Planet Imager (GPI) instrument. Direct imaging of extrasolar planets separates the light of the (faint) planet and (bright) star, allowing us to measure the spectrum of young self-luminous giant exoplanets.

Chao-Lin’s group use the most ancient light, the Cosmic Microwave Background (CMB) radiation, emitted when the universe was in its infancy to shed light on the question of how the universe began. Currently Chao-Lin's group are involved in a number of experiments such as BICEP/BICEP2/Keck Array and have been working hard on detecting primordial B-mode polarization. His group are involved in both he design and construction of instruments as well as the data analysis and theoretical interpretation.