Vuk Mandic

man wearing brown jacket

Vuk Mandic

Professor, School of Physics and Astronomy

Contact

Physics And Nanotechnology Building
Room 328
115 Union St. Se
Minneapolis, MN 55455

Affiliations

Minnesota Institute for Astrophysics (MIfA)

Education

Ph.D., University of California, Berkeley, 2004

B.S., Caltech, 1998

Professional Background

Chair of the SuperCDMS Non-project R&D Working Group, 2014-present

Chair of the SuperCDMS Elections and Appointments Committee, 2012-2015

Member of the LIGO Calibration Review Committee, 2006-2013, Chair 2009-2013

Member of the LSC-VIRGO Data Analysis Council, 2007-2011

Co-chair of the Stochastic Working Group of the LIGO Scientific Collaboration (LSC), 2006-2011

Member of the LSC Data Analysis Committee, 2006-2007

Research Interests

My research focuses on the physics of the earliest stages of the Universe and of the highest energies. In particular, I am interested in experiments that probe content and properties of the Universe today, and that can shed light on the evolution of the Universe and on the physics at high energy scales. I work on two such experiments.

Gravitational Wave Search: LIGO

Laser Interferometer Gravitational-wave Observatory (LIGO) has built multi-kilometer interferometers at two sites: Hanford, WA and Livingston Parish, LA. These interferometers are designed to search for gravitational waves that could be produced in some of the most violent events in the Universe: mergers of two neutron stars or black holes, supernova explosions, or the Big Bang. Detection of gravitational waves would therefore open a new window into astrophysics and could potentially give us a view of the very early Universe, when the Universe was only a fraction-of-a-second old.

The gravitational wave detectors are sensitive to motions at the level of one ten-thousandth of the proton size. Much of my work is geared toward understanding and suppressing the contributions from various noise sources that are important at such sensitivities. Currently we are focusing on the seismic noise and on the Newtonian noise (fluctuations in the local gravitational field due to the motion of nearby masses). I lead an interdisciplinary project known as the Deep Underground Gravity Lab (DUGL) at the Homestake mine, SD, where we are developing a unique 3D array of seismometers with the goal of understanding the behavior of the seismic noise underground. While our main motivation comes from the field of gravitational waves, the DUGL project is also of substantial interest in geophysics and is therefore conducted in collaboration with geophysicists.

My group is also involved in searches for the stochastic background of gravitational waves using LIGO data. The origin of such a background could be cosmological (inflationary models, cosmic strings models) or astrophysical (integrating supernovae or pulsar signals across the Universe). We have placed the most stringent bounds on the energy density in gravitational waves and we have produced the first (upper limit) maps of the gravitational-wave sky, thereby constraining some of the models of stochastic gravitational-wave background. We are also pursuing searches for gravitational wave transients on the scale of minutes, hours, or longer. We expect all of these searches to make substantial advances in the next 3-5 years, taking advantage of the new, more sensitive data from Advanced LIGO (coming online in September 2015), and potentially resulting in the first detections of gravitational waves.

Dark Matter Search: CDMS

Together with Prof. P. Cushman, I am involved in the Super Cryogenic Dark Matter Search (SuperCDMS) experiment, which is designed to search for dark matter in the form of new particles, generically called Weakly Interacting Massive Particles (WIMPs). There is an overwhelming evidence today that most of the matter in the Universe is invisible (i.e. dark), and most likely non-baryonic. However, the nature of dark matter is presently unknown, turning it into one of the most pressing problems in cosmology today. WIMPs represent one possible solution to the dark matter problem. They are particularly interesting because they naturally appear in supersymmetry and large extra-dimensions models - hence, discovery of WIMPs could have far-reaching implications for particle physics, in addition to solving the dark matter problem.

SuperCDMS has designed detectors based on crystals of germanium or silicon, operated at very low temperatures (30-50 mK), and in very low background conditions (deep underground in the Soudan mine, MN, with substantial shielding). These detectors are capable of identifying and rejecting the known particle backgrounds very efficiently, hence allowing a measurement of a signal due to a new particle (WIMP). CDMS has been at the forefront of the WIMP searches over the past decade, and will remain at the forefront with the approved second-generation experiment SuperCDMS-SNOLab. My research focus within CDMS is development and characterization of detectors in our cryogenic laboratory, mostly geared toward increasing the detector size which would simplify scaling up the total mass of the experiment. My group is also heavily involved in the analysis of CDMS data.

Research Group
Super Cryogenic Dark Matter Search (SuperCDMS)
Laser Interferometer Gravitational-wave Observatory (LIGO)
Deep Underground Gravity Lab (DUGL)

Honors and Awards

McKnight Professorship, 2010-2012

Selected Publications

  1. The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration, Search for anisotropic gravitational-wave backgrounds using data from Advanced LIGO's and Advanced Virgo's first three observing runsarXiv:2103.08520 (2021).

  2. S.Banagiri et al, Mapping the Gravitational-wave Sky with LISA: A Bayesian Spherical Harmonic Approach, arXiv:2103.00826 (2021)

  3. The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration, Upper Limits on the Isotropic Gravitational-Wave Background from Advanced LIGO's and Advanced Virgo's Third Observing RunarXiv:2101.12130 (2021).

  4. K.Z. Yang et al, Searching for Cross-Correlation Between Stochastic Gravitational Wave Background and Galaxy Number CountsMon. Notices Royal Astron. Soc. 500.2, 1666 (2021).

  5. S. Banagiri et al, Measuring angular N-point correlations of binary black hole merger gravitational-wave events with hierarchical Bayesian inference, Phys. Rev. D 102, 063007 (2020).

  6. The LIGO Scientific Collaboration and Virgo Collaboration, GW190521: A Binary Black Hole Merger with a Total Mass of 150 Msun, Phys. Rev. Lett. 125, 101102 (2020).

  7. M. Coughlin et al.Coherence-based approaches for estimating the composition of the seismic wavefield, J. Geophys. Res.: Solid Earth 124, 2941 (2019).

  8. P. Meyers et al, Direct Observations of Surface‐Wave Eigenfunctions at the Homestake 3D Array, Bull. Seism. Soc. Amer. 109, 1194 (2019).

  9. The LIGO Scientific Collaboration and Virgo Collaboration, All-sky search for long-duration gravitational wave transients in the second Advanced LIGO observing run, Phys. Rev. D 99, 104033 (2019).

  10. The LIGO Scientific Collaboration and Virgo Collaboration, Directional limits on persistent gravitational waves using data from Advanced LIGO's first two observing runs, Phys. Rev. D 100, 062001 (2019).