Tuesdays at 4:00 PM in the Marlar Lounge, Room 37-252
MIT Kavli Institute for Astrophysics and Space Research
70 Vassar Street, Cambridge, MA
(unless location otherwise noted)
Refreshments are served at 3:45 PM.
the Astrophysics Division of the MIT Department of Physics and
the MIT Kavli Institute for Astrophysics and Space Research.
Tuesday Feb 7:
Cosmology with Shadows in the Microwave Sky
Host: M. McDonald
Our current 6-parameter LambdaCDM cosmological model is well
constrained by observations in the linear regime, such as measurements
of the cosmic microwave background (CMB) radiation. A new frontier for
cosmology is to search for departures from this model, which pushes
future measurements into the non-linear regime (e.g., late-time growth
of structure). The thermal Sunyaev Zel'dovich (tSZ) effect offers a
unique way to probe the growth of structure using high-resolution CMB
experiments, such as the Atacama Cosmology Telescope. I will review
the recent tSZ cosmological constraints and discuss the astrophysical
uncertainties that currently limit them. I will discuss current
efforts to mitigate these astrophysical uncertainties highlighting the
role that optical surveys like the Large Synoptic Survey Telescope
will play. I will describe the prospects for future CMB experiments
like the Simons Observatory and CMB-S4 to constrain departure from our
standard cosmological model with tSZ observations.
Tuesday Feb 14:
New Probes of Old Structure: Cosmology with 21cm Intensity Mapping and the Cosmic Microwave Background
Host: J. Hewitt
Current cosmological measurements have left us with deep questions about our Universe: What caused the expansion of the Universe at the earliest times? How did structure form? What is Dark Energy and does it evolve with time? New experiments like CHIME, HIRAX, and ACTPol are poised to address these questions through 3-dimensional maps of structure and measurements of the polarized Cosmic Microwave Background. In this talk, I will describe how we will use 21cm intensity measurements from CHIME and HIRAX to place sensitive constraints on Dark Energy between redshifts 0.8 -- 2.5, a poorly probed era corresponding to when Dark Energy began to impact the expansion history of the Universe. I will also discuss how we will use data from new instruments on the ACT telescope to constrain cosmological parameters like the total neutrino mass and probe structure at late times.
Tuesday Feb 21:
Tracing the Cosmic Shutdown of Star Formation in Massive Galaxies
University of Connecticut
Host: M. Vogelsberger
Over the last few decades, astronomers have progressed from archeological studies of nearby galaxies to direct observations of the early universe. We have uncovered billions of years of cosmic growth that present new challenges to galaxy formation theories. In this talk, I will review the recent innovative techniques developed to probe the distant universe, and the key observations constraining the formation histories of galaxies over the past 11 billion years. We have discovered a population of surprisingly compact and massive “red and dead” (quiescent) galaxies that are no longer actively forming stars. The physical mechanisms responsible for shutting down star formation and the subsequent buildup of this quiescent population at such early times is one of the most outstanding questions in astrophysics today. We don’t yet understand why these enigmatic galaxies are so compact, with sizes a factor of 5 smaller than nearby galaxies of similar mass. I will present promising paths forward towards solving this puzzle that leverage the capabilities of the Hubble Space Telescope, as well as a look toward the future with exciting upcoming public facilities.
Tuesday Feb 28:
The Physics and Astrophysics of Merging Neutron-Star Binaries
Goethe University of Frankfurt
Host: S. Hughes
I will argue that if black holes represent one the most fascinating implications of Einstein's theory of gravity, neutron stars in binary system are arguably its richest laboratory, where gravity blends with astrophysics and particle physics. I will discuss the rapid recent progress made in modelling these systems and show how the inspiral and merger of a binary system of neutron stars is more than a strong source of gravitational waves. Indeed, while the gravitational signal can provide tight constraints on the equation of state for matter at nuclear densities, the formation of a black-hole--torus system can explain much of the phenomenology of short gamma-ray bursts, while the ejection of matter during the merger can shed light on the chemical enrichment of the universe.
Tuesday Mar 7:
Stellar Streams and the Milky Way's Dark Matter Halo
University of Toronto
Host: P. Schechter
Stellar tidal streams originating from disrupting globular clusters in the Milky Way's halo hold enormous promise as probes of both the large-scale structure of the Milky Way halo's density distribution and its small-scale structure. As such, the observed density, spatial, and kinematic structure of stellar streams can provide important new constraints on the interactions and small-scale structure of dark matter. I will discuss the simple gravitational dynamics of tidal-stream formation and evolution and how we can use it to build simple and fast models for tidal streams. I will show some examples of this machinery in fitting observed streams and what it tells us about the shape of the Milky Way's halo. I will further present a fast perturbation theory for computing the effects of impacts between a stream and many small dark-matter subhalos and its application to existing and future data sets.
Tuesday Mar 14:
Imaging All the Sky All the Time in Search of Radio Exoplanets
Host: M. McDonald
All the magnetized planets in our solar system, including Earth, produce bright emission at low radio frequencies, predominantly originating in high magnetic latitudes and powered by auroral processes. It has long been speculated that similar radio emission may be detectable from exoplanets orbiting nearby stars, which would provide the first direct confirmation of the presence, strength and extent of exoplanetary magnetospheres, as well as informing on their role in shielding the atmospheres of potentially habitable exoplanets. Despite 4 decades of observations, no detection has been achieved. Surprisingly, however, brown dwarfs have been found to produce both radio and optical emissions that are strikingly similar to the auroral emissions from solar system planets, albeit 10,000 times more luminous, bolstering the continued search for similar emission from exoplanets. In the case of the latter, the absence of detection thus far may simply be due to the highly variable nature of the radio emission. The auroral radio emission from Earth can increase by three orders of magnitude during a geomagnetic storm and a similar dependence on local space weather conditions can be assumed for exoplanets, requiring dedicated monitoring of stellar systems to enable detection. I will discuss the auroral radio emission from exoplanets and brown dwarfs and introduce a new radio telescope, consisting of 352 antennas spaced across 2.5 km, that images the entire viewable sky every ten seconds at low radio frequencies, thereby monitoring thousands of stellar systems simultaneously in the search for radio emission from exoplanets.
Tuesday Mar 21:
Dark Matter Substructure: Cosmological Treasure Trove or a Pandora's Box?
Frank van den Bosch
Host: P. Schechter
Hierarchical structure formation in a LCDM cosmology gives rise to virialized
dark matter halos that contain a wealth of subtructure. Being able to accurately
predict the abundance and demographics of dark matter subhaloes is of paramount
importance for many fields of astrophysics: gravitational lensing, galaxy evolution,
and even constraining the nature of dark matter. Dark matter substructure is
subject to tidal stripping and tidal heating, which are highly non-linear processes
and therefore best studied using numerical N-body simulations. Unfortunately, as I
will demonstrate, state-of-the-art cosmological simulations are unable to adequately
resolve the dynamical evolution of dark matter substructure. They suffer from a
dramatic amount of artificial subhalo disruption as a consequence of both inadequate
force softening and discreteness noise amplification in the presence of a tidal field.
I discuss implications for a variety of astrophysical applications, and briefly
discuss potential ways forward.
Tuesday Mar 28:
NO COLLOQUIUM: SPRING VACATION
Tuesday Apr 4:
Probing New Physics with the Cosmic Microwave Background
University of Chicago
Measurements of the Cosmic Microwave Background (CMB) have been extremely important for our understanding of the origin, contents, and evolution of the universe. Increasingly precise maps of the CMB are a unique and powerful tool for understanding new physics, including inflation, the superluminal expansion of the universe during the first moments after the Big Bang. I will discuss the current status of CMB measurements, focusing on constraints on inflation with the BICEP series of experiments at the South Pole (BICEP2, The Keck Array, and BICEP3). I will then discuss the rapidly moving plans for a next-generation ground-based program called CMB-S4. The sensitivity leap of CMB-S4 is needed to pass critical thresholds in our understanding of inflation, neutrino mass, and in searches for additional light relativistic species.
Tuesday Apr 11:
Synergy of molecular clouds and a supermassive black hole in our Galactic Center.
Max Planck Institute für Astrophysik
Host: C. Canizares
While the supermassive black hole Sgr A* at the center of the Milky Way is currently very dim, we believe that it experienced a powerful outburst of X-ray radiation hundreds of years ago. The historical records of this outburst are revealed by reflection/reprocessed radiation coming from dense molecular clouds. The imprints left by the outburst in spatial and time variations of the reflected emission suggest that the outburst happened some hundred years ago. It lasted less than several years and Sgr A* was about hundred million times brighter than today. These characteristics are consistent with a relatively modest tidal disruption event. Thus, molecular clouds offer us a convenient tool to study Sgr A*’s past history. At the same time, the outburst serves as an extremely powerful probe of molecular gas. Essentially, this is the only opportunity to reconstruct a full 3D structure of molecular clouds and their mass distribution. Future X-ray observatories, including cryogenic bolometers and polarimeters, will further boost our ability to conduct in-depth studies of molecular gas and outbursts of Sgr A*.
Tuesday Apr 18:
NO COLLOQUIUM: PATRIOT'S DAY
Tuesday Apr 25:
University of Bern
Host: N. Weinberg
Tuesday May 2:
University of Washington
Host: S. Vitale
Tuesday May 9:
Host: D. Chakrabarty
Tuesday May 16:
Scuola Normale Superiore
Host: J. Hewitt