Joint IAS Princeton University Astrophysics Colloquium
Fall 2021 Colloquium Series
The Fall 2021 Joint Astrophysics Colloquium will be held on Tuesdays at 11AM and will be followed by the Bahcall Lunch at 12:30.
Please find the Fall speaker schedule at this link and below. Videos on IAS website: https://www.ias.edu/video-tags/iaspu-joint-astrophysics-colloquium
|Date||Name||Title (link to videos of talks is here.)|
|Sep 7 11:00am||Romain Teyssier||Cosmic magnetism from a computational perspective|
|Sep 14 11:00am||Alice Quillen||Soft Astronomy|
|Sep 21 11:00am||Amina Helmi||New views on the Milky Way|
|Sep 28 11:00am||Uros Seljuk||All you need is a Normalizing Flow|
|Oct 5 11:00am||Brett McGuire||The PAH Revolution: Cold, Dark Carbon at the Earliest Stages of Star Formation|
|Oct 12 11:00am||Jennifer Lotz||Gemini Observatory in the 2020's|
|Oct 26 11:00am||Ellen Zweibel||TBA|
|Nov 2 11:00am||Xuening Bai||TBA|
|Nov 9 11:00am||Kenta Kiuchi||TBA|
|Nov 16 11:00am||Sera Markoff||TBA|
|Nov 23 11:00am||Alexandra Amon||TBA|
|Nov 30 11:00am||Bethany Ehlmann||TBA|
2021 Summer Colloquium Series
The 2021 Summer Colloquium Series led by Professor Eliot Quataert begins virtually on
Wed. Jul 21, at 12:00PM, and continues on Tuesdays 7/27 through 8/24 at 12:30PM.
The list of speakers, talk titles and select colloquium recording links appear below. Zoom link will be sent by email.
|Date||Name||Title (Video Link to Talk)|
|July 21, 2021
|Unraveling The Universe With Cosmic Voids
Modern surveys provide access to high-quality measurements on large areas of the sky, sampling the galaxy distribution in detail also in the emptiest regions, voids. Void cosmology is becoming an increasingly active sector of galaxy clustering analysis: by measuring void properties, such as density profiles or void number counts, it is possible to constrain cosmological parameters. Cosmic voids are particularly sensitive to the properties of dark energy and neutrinos, and are a powerful tool to test modifications of the laws of general relativity. Studying voids provides a novel perspective to unravel the unsolved mysteries of our Universe.
In this talk I introduce cosmic voids as a tool for cosmology, I present recent results—with a particular focus on the advantages of calibration-free approaches—and I discuss future developments in the field.
|July 27, 2021
|Kirk Barrow Stanford||High-Cadence Synthetic Observations and Neural Networks in the Era of JWST
As astronomers near the commissioning of the extremely large telescopes, the Rubin Observatory, as well as new space-based observatories like the Roman Space Telescope and JWST to peer more deeply into our Universe, our community is challenged to develop a theoretical and modeling framework to characterize and study what will be humanity's greatest astronomical discoveries. My research addresses this need by generating detailed, state-of-the-art synthetic observations from hydrodynamic cosmological simulations. By calculating all the processes that photons undergo as they travel across the Universe from the surface of a distant star to a telescope’s detector, my collaborators and I have been able to disentangle perplexing trends in observed galactic spectra as well as make predictions for what we might unveil in the near future. Topics we have investigated in prior work include massive black hole formation, the first stars and galaxies, and the intricate interplay between nebular emission lines and the escape fraction of ionizing radiation. Looking forward, I propose to create the largest and most detailed database of synthetic observational tools and predictions at a time that will come to define astronomy for generations.
|Aug. 3, 2021
|Microphysical Insights into Protoplanetary Disks and Exoplanet Atmospheres
A fundamental understanding of planetary histories and characteristics requires an empirical connection between planet formation and evolved planets—a long-sought goal of astrophysics. This connection is now increasingly possible due to simultaneous revolutions in the observations of protoplanetary disks and exoplanet atmospheres. A key step towards relating these observations of different evolutionary stages is to characterize the composition of material in protoplanetary disks and relate these properties to the atmospheric composition of planets. In this talk, I will discuss initial steps that I have taken towards this goal. I will provide evidence that protoplanetary disks are more than an order of magnitude more massive than previously appreciated, that the detailed properties of clouds shape observations of substellar atmospheres, and that the physics of modeling clouds gives a new understanding of the compositional distribution in protoplanetary disks. I will conclude by briefly discussing avenues for relating planetary properties to the mass inventory in protoplanetary disks in order to develop the observationally-validated framework required to compositionally relate evolved planets to planet formation.
|Aug. 10, 2021
|Understanding Planetary Evolution with Eclipsing Disks & Transiting Planets
The success of ground-based transit and RV surveys, and the Kepler/K2 and TESS missions, have shifted the exoplanet field from pure discovery to a combination of discovery, demographic analysis, and detailed characterization, especially for exoplanet atmospheres. We are using data from the TESS, Kepler/K2, and ground-based transit surveys to find keystone planetary systems around bright stars (those well suited for atmospheric observations) that can help address specific questions about planet formation and evolution. We are also studying the birthplaces of planets by searching for occultations of newly formed stars by their protoplanetary disks. These systems provide insight into the conditions required for planet formation. I will describe our recent results from both projects and discuss how we will study these types of objects in future surveys.
|Aug. 24, 2021
|First-Principles Modeling of Kinetic Turbulence in High-Energy Astrophysical Plasmas
Kinetic plasma physics is an integral, but often neglected, component of many high-energy astrophysical systems. Understanding the dynamics and energization processes in collisionless plasmas is essential for interpreting the observable radiation spectra, luminosities, and variability of systems such as pulsar wind nebulae, accretion flows onto compact objects, and relativistic jets from active galactic nuclei. Kinetic turbulence has long been proposed as a primary process for energizing these collisionless plasmas, but questions remain as to its viability for producing nonthermal particle populations in various physical regimes. Particle-in-cell (PIC) simulations have recently opened this rich topic to detailed, first-principles numerical and theoretical scrutiny. I will overview recent progress on understanding particle energization in relativistic (and trans-relativistic) plasma turbulence, spurred by PIC simulations, including the demonstration of phenomena such as nonthermal particle acceleration, electron-ion thermal decoupling, and intermittent beaming of radiation. These new insights have applications for modeling various high-energy astrophysical systems.
2021 Spring Colloquium Series
The Spring 2021 Joint Astrophysics Colloquium was held virtually on Tuesdays at 11AM and was followed by the virtual Bahcall Lunch at 12:30.
|Date||Name||Title (Video Link to Talk) (pvt)|
|Feb. 2, 2021||Eliot Quataert
|The Impact of Cosmic-Rays on Galaxy Formation
Relativistic cosmic-rays created by stellar and black hole feedback may play an important role in many aspects of structure formation. Cosmic-rays can drive outflows from star forming galaxies and heat diffuse gas in the circumgalactic and intergalactic medium. In this talk I will describe some of the possible impact(s) of cosmic-rays on galaxy formation, observational probes of their impact, and the
theortical uncertainities in our understanding of the role of cosmic rays in structure formation.
|Feb. 9, 2021||Feryal Özel
University of Arizona
|Black Hole Physics at the Horizon Scale
Recent observational advances with the Event Horizon Telescope, GRAVITY, and LIGO/VIRGO have opened up new avenues for studying black hole physics at horizon scales. In this talk, I will discuss what we have learned about the spacetimes of astrophysical black holes and how strong-field gravity is imprinted on their images. I will also present how the observations help us model and understand the heating and acceleration of plasmas on horizon scales.
|Feb. 16, 2021||Sherry Suyu
Max Planck Institute for Astrophysics
|Cosmology with Gravitational Lens Time Delays
Strong gravitational lenses with measured time delays between the multiple images can be used to determine the Hubble constant (H0) that sets the expansion rate of the Universe. An independent determination of H0 is important to ascertain the possible need of new physics beyond the standard cosmological model, given the tension in current H0 measurements. I will describe techniques for measuring H0 from lensing with a realistic account of systematic uncertainties, and present the latest results from a program aimed to measure H0 from lensing. Search is underway to find new lenses in imaging surveys. An exciting discovery of the first strongly lensed supernova offered a rare opportunity to perform a true blind test of our modeling techniques. I will show the bright prospects of gravitational lens time delays as an independent and competitive cosmological probe.
|Feb. 23, 2021||Jørgen Christensen-Dalsgaard
|Probing red giants with Kepler
The frequencies of oscillations observed on a stellar surface carry information about the properties of the stellar interior. Asteroseismology, i.e., the unravelling of this information, has made a huge leap thanks to the photometric observations obtained with NASA' Kepler mission, launched in 2009 to search for planets around other stars. In my talk I focus on the study of red-giant stars, showing a broad range of oscillations, probing both the outer parts and the deep core of the stars. Amongst other remarkable results, this has allowed distinguishing stars according to their nuclear energy source and provided detailed information about the properties of internal rotation in these late stages of stellar evolution.
|Mar. 2, 2021
|Jennifer van Saders
University of Hawaii
|Making Sense of Stellar Rotation in Low Mass Stars
Stellar rotation carries a wealth of information about stellar populations. In particular, the technique of gyrochronology was developed to utilize the spin-down of stars as a function of time as an indicator of stellar age. Gyrochronology has the potential to yield precise ages for large samples of stars, providing unprecedented chronological information for studies of the Milky Way and extrasolar planets. However, the technique is in its adolescence: it has been tested and validated under limited scenarios, but its weaknesses and limitations have hitherto been largely unexplored. With time-domain data we can address these gaps: we now have access to datasets of rotation periods for tens of thousands of stars, as well as independent asteroseismic ages and rotation periods for a few hundred old (main sequence) stars. I will discuss my comparisons of theoretical rotation models to these data, which have yielded unexpected insights into the rotational and magnetic lives of stars (and the Sun!), as well as a better understanding of the power and peril of gyrochronology as a tool.
|Mar. 16, 2021||Brian Nord
University of Chicago / Fermilab
|From Galaxies to Faces: Recognizing the Implications of Artificial Intelligence in Astronomy and Society
Artificial Intelligence (AI) refers to a set of techniques that rely primarily on the data itself for the construction of a quantitative model. AI has arguably been in development for three quarters of a century, but there has been a recent resurgence in research and application. This current (third) wave of AI progress is marked by extraordinary results --- for example, in image analysis, language translation, and machine automation. Despite the aforementioned modest definition of AI, its potential to disrupt technologies, economies, and society is often presented as (nearly) unmatched in modern times, due in part to the versatility of the algorithms in modeling a wide variety of data. Similarly, there is great promise for applications across the sciences --- for example, simulations, image classification, and automated experimentation --- which are currently being investigated by researchers across the globe. Along with the significant promise of AI, comes great peril: in societal contexts, the consequences include enhanced surveillance, facial recognition, and automated weaponry. In science contexts, the issues are also significant and in many cases related --- for example, bias, lack of uncertainty quantification, and misuse. To take full advantage of the opportunities for AI to accelerate science and improve society, it's essential that we carefully guide its development.
During this presentation, we will explore modern AI techniques, like neural networks, and review how they are being developed and deployed in astronomy. Then, we’ll discuss ideas for the future usage of AI in science, including technical barriers for long-term application. Finally, we’ll discuss the roles of scientists and academic communities in the development of AI algorithms
|Mar. 23, 2021||Julia Roman-Duval
Space Telescope Science Institute
|The Nearby Universe - A Laboratory to Study the Cosmic Build-up of Dust and Metals in Galaxies
A key component of the baryon cycle in galaxies is the cycle of metals between the gas and the dust phases in the neutral interstellar medium (ISM). How this cycle depends on environment (in particular metallicity and density) has important implications for how accurately we can trace the chemical enrichment of the universe over cosmic times; either by using dust emission in the far-infrared as a tracer of the ISM in galaxies at high and low redshift; or by using spectroscopy of damped Lyman-alpha systems (DLAs) to measure chemical abundances in neutral gas over a wide range of redshifts. Variations of the abundance and properties of dust within and between galaxies furthermore profoundly affects their evolution, given the key role that dust plays in the chemistry, radiative transfer, and thermodynamics of galaxies. In this talk, I will present results from several independent observational efforts to characterize the dust abundance (dust-to-gas and dust-to-metal ratios) in the Magellanic Clouds and other nearby low-metallicity galaxies, using emission-based tracers of the interstellar medium (FIR, HI 21 cm, CO rotational emission) to map their dust and gas content on the one hand; and using UV absorption spectroscopy with Hubble to directly count metals in the gas phase on the other hand. Both types of studies demonstrate significant variations of the dust abundance with density (within galaxies) and metallicity (between galaxies), which have important implications for the sub-grid physics of galaxy evolution. Surprising patterns in the gas-phase abundances were found from the Hubble spectroscopy, and an interesting tension between the emission-based and absorption-based measurements remains unexplained.
|Mar. 30, 2021||Anna Watts
University of Amsterdam
|A NICER view of neutron stars
NICER, the Neutron Star Interior Composition Explorer, is an X-ray telescope that was installed on the International Space Station in 2017. Its mission is to study the nature of the densest matter in the Universe, found in the cores of neutron stars. NICER uses Pulse Profile Modeling, a technique that exploits relativistic effects on X-rays emitted from the hot magnetic polar caps of millisecond pulsars. The technique also lets us map the hot emitting regions, which form as magnetospheric particles slam into the stellar surface. I will present NICER's current results and ongoing analysis, and discuss the implications for our understanding of ultradense matter, pulsar emission, and stellar magnetic fields.
|Apr. 6, 2021||Zhaohuan Zhu
University of Nevada, Las Vegas
|Protoplanetary Disk Structure and Young Planet Population
Recent ground based observations at various wavelengths reveal a variety of protoplanetary disk structures. These disk structures may help us to constrain the planet formation process. I will first discuss how to apply the planet-disk interaction theory to substructures in the ALMA DSHARP sample to reveal the potential young planet population. We find that the occurrence rate for >5 M J planets beyond 5-10 au is consistent with direct imaging constraints. Disk substructures allow us to probe a wide-orbit planet population (Neptune to Jupiter mass planets beyond 10 au) that is not accessible to other planet searching techniques. On the other hand, ALMA surveys have suggested that the dust in Class II disks may not be enough to explain the averaged solid mass in exoplanets, under the assumption that the mm disk continuum emission is optically thin. I will question this optically thin scenario and point out that dust scattering can considerably reduce the emission from an optically thick region. This optically thick disk scenario can solve several puzzles in protoplanetary disk observations and can provide enough dust to form exoplanets. Finally, I will talk about my ongoing work on 3-D radiation hydrodynamical simulations of forming Jupiter’s convective envelope.
|Apr. 13, 2021||Yamila Miguel
|Unveiling the secrets of Jupiter with the Juno mission
With more than 4000 exoplanets found and about 2-dozens of planets with detected atmospheric chemical species, we moved from an era of discovery to a new era of exoplanet characterisation. On the other hand, extremely accurate measurements by Juno and Cassini missions, make this an exceptional time to combine the detail information on the solar system giant planets and the large amount of data from exoplanets to get a better understanding on planetary physics and a better comprehension on planet formation and evolution.
Because our knowledge on the interior structure of the giant planets is linked with the data we obtain from space missions, these last years were crucial for this field: the outstanding accuracy of the gravity data provided by Juno has fundamentally changed our understanding of the interior of Jupiter. It has allowed us to put constrains on the zonal flows, the extent of differential rotation and lead us to find that Jupiter has most likely a dilute core. In this presentation I will review our knowledge on the interior structure of Jupiter and will also show some new results where we find that a non-homogenous envelope is also a constraint set up by the Juno measurements, which is helping us to get closer to unveiling Jupiter’s deep secrets and to reach a better understanding of the giant planets formation history.
|Apr. 20, 2021||Ignas Snellen
|Exoplanets and the search for extraterrestrial life
Abstract: Placing the solar system in the context of other planetary
systems is one of the central objectives driving the study of extrasolar
planets. One of the most fascinating questions in modern science is
whether other life-bearing planets exist. In this talk I will review the
current state of the art of exoplanet research and discuss future ways
to probe biomarker gases in Earth-like exoplanets that could point to
|Apr. 27, 2021||Alberto Bolatto
University of Maryland
|The Inner Workings of Starbursts
Starbursts are a rare phenomenon in the present day universe, but they represent perhaps the most common mode under which stars form and galaxies grow during the z~1-2 peak of cosmic star formation activity. This mode of star formation is not a simple scaling of what happens in typical molecular clouds, but represents a much more efficient manner of converting gas into stars likely through the formation of massive clusters. The resulting feedback in the form of galaxy-scale outflows is, together with AGN, thought to be one of the main forms of regulation of galaxy growth. I will show the analysis of recent, high resolution observations of three of the nearest starbursts: NGC253, NGC4945, and M82. I will first discuss the properties of their galactic molecular outflows, including our best constraints on the mass and outflow rate, and the properties of the molecular gas. Then I will focus on the results from high-resolution observations which reveal a dozen compact structures with properties corresponding to massive young star clusters and super star clusters (SSCs), most of which are so embedded that are invisible in optical and NIR observations. Finally, I will present the analysis of 0.5-pc resolution observations of NGC253 which reveal feedback and disruption on the scales of these clusters, I will discuss the properties of these "cluster-scale" outflows, and I will compare them to theoretical expectations.
2020 Fall Colloquium Series
The Fall 2020 Joint Astrophysics Colloquium was held virtually on Tuesdays at 11AM and was followed by the Bahcall Lunch at 12:30, also virtual.
Please find the Fall speaker schedule here. Videos of the talks can be found on the IAS website: https://www.ias.edu/video-tags/iaspu-joint-astrophysics-colloquium
2020 Summer Colloquium Series
The 2020 Summer Colloquium Series led by Professor Jenny Greene has concluded. The list of speakers, talk titles and select colloquium recording links appear below.
|Jun 30, 2020||Evan Schneider||The Origin of Multiphase Galaxy Outflows|
|July 7, 2020||Courtney Dressing||Exploring Planets Orbiting Nearby Stars|
|July 14, 2020||Geraldine Cochran||Promoting Diversity and Addressing Barriers in Physics|
|July 21, 2020||Sean Johnson||Observations of the gas flows that govern galaxy evolution in absorption and emission at z<1|
|July 28, 2020||Julie Posselt||Equity in Science: Representation, Culture, and the Dynamics of Change in Graduate Education|
|Aug 4, 2020||Richard Anantua||A Glimpse into Horizon-Scale Physics Using Movies and Polarization Maps|
|Aug 11, 2020||Casey Miller||Practicing Equity in Graduate Admission|
|Aug 25, 2020||Kareem El-Badry||Emission-line stars, binary mass transfer, and the search for detached stellar mass black hole|