Member-at-large of APS Topical Group on Gravitation
Just one more committee
Just one more committee
Angular momentum is tricky to define in GR! Here’s an approach so that observers can all agree with each others’ measurements.
The first astrophysically-relevant numerical simulation of merging black holes in a higher-curvature theory beyond GR.
The first numerical beyond-GR binary black hole merger simulation.
Want to hear me talk about numerical relativity and theories beyond GR?
Finding the shape of extremal black holes in beyond-GR theories
Here to save you some algebra and column-inches
Just an update on talks I gave recently. Valeria Ferrari, Leonardo Gualtieri, and Paolo Pani hosted the conference “New Frontiers in Gravitational-Wave Astr...
One of the first numerical simulations of black hole mergers in beyond-GR effective field theories
My talk slides/movies from TG17 and APS17
My talk slides/movies from the FF2016 conference at Northwestern
My talk slides/movies from the GR21 conference in NYC
My talks slides/movies from the 2016 April APS meeting in SLC
Progress in understanding the structure of extremal black holes in Chern-Simons
Numerical solutions for rapidly-rotating dCS black holes show where the weak-coupling expansion breaks down.
Just one more committee
In theories of gravity that include a scalar field, a compact object’s scalar charge is a crucial quantity since it controls dipole radiation, which can be s...
Finding the shape of extremal black holes in beyond-GR theories
Here to save you some algebra and column-inches
Not all theories with long-ranged scalar fields produce dipole radiation in binaries
I missed the author index from LRR, so I rebuilt one.
Gravity theories beyond general relativity (GR) can change the properties of gravitational waves: their polarizations, dispersion, speed, and, importantly, e...
I hosted a Quora session. It went well!
I missed the author index from LRR, so I rebuilt one.
A surrogate model extending the parameter space range of fully precessing quasicircular inspirals
Accurate models of gravitational waves from merging black holes are necessary for detectors to observe as many events as possible while extracting the maximu...
Sometimes in a numerical method, you need to be able to continuously turn a calculation on or off in space or time.
Interactive toy for visualizing relationship between polynomial roots and coefficients
Here to save you some algebra and column-inches
An identity between vector commutation coefficients and coframe connection coefficients
These three objects form a superalgebra! Whoa!
There is a nice 4-dimensional Weyl identity that I can never seem to remember off the top of my head; so I decided I need to write this note so I don’t have ...
Angular momentum is tricky to define in GR! Here’s an approach so that observers can all agree with each others’ measurements.
The first astrophysically-relevant numerical simulation of merging black holes in a higher-curvature theory beyond GR.
The first numerical beyond-GR binary black hole merger simulation.
Want to hear me talk about numerical relativity and theories beyond GR?
Gravity theories beyond general relativity (GR) can change the properties of gravitational waves: their polarizations, dispersion, speed, and, importantly, e...
In theories of gravity that include a scalar field, a compact object’s scalar charge is a crucial quantity since it controls dipole radiation, which can be s...
Finding the shape of extremal black holes in beyond-GR theories
Here to save you some algebra and column-inches
Just an update on talks I gave recently. Valeria Ferrari, Leonardo Gualtieri, and Paolo Pani hosted the conference “New Frontiers in Gravitational-Wave Astr...
One of the first numerical simulations of black hole mergers in beyond-GR effective field theories
My talk slides/movies from TG17 and APS17
My talk slides/movies from the EHT16 conference in Cambrige, MA
My talk slides/movies from the FF2016 conference at Northwestern
My talk slides/movies from the GR21 conference in NYC
My talks slides/movies from the 2016 April APS meeting in SLC
Invited review for CQG Focus Issue
Progress in understanding the structure of extremal black holes in Chern-Simons
Not all theories with long-ranged scalar fields produce dipole radiation in binaries
A major review on non-GR theories, black holes and neutron stars in non-GR theories, compact binaries in non-GR theories, and pulsar, gravitational-wave, and...
Numerical solutions for rapidly-rotating dCS black holes show where the weak-coupling expansion breaks down.
MIT PhD thesis of Leo C. Stein
The dividing line between bound and plunging orbits is an algebraic variety
The first astrophysically-relevant numerical simulation of merging black holes in a higher-curvature theory beyond GR.
qnm is an open-source Python package for computing the Kerr quasinormal mode frequencies, angular separation constants, and spherical-spheroidal mixing coeff...
Hear me, Katie Bouman, and friends talk about how to snap a picture of a black hole with the Event Horizon Telescope!
The first numerical beyond-GR binary black hole merger simulation.
A surrogate model extending the parameter space range of fully precessing quasicircular inspirals
Accurate models of gravitational waves from merging black holes are necessary for detectors to observe as many events as possible while extracting the maximu...
I’m on Episode 42 of the Starts with a Bang Podcast
Want to hear me talk about numerical relativity and theories beyond GR?
Real-time interactive visualizations of merging black holes in seconds!
Modeling black holes remnants directly from numerical relativity
In theories of gravity that include a scalar field, a compact object’s scalar charge is a crucial quantity since it controls dipole radiation, which can be s...
Modeling black holes’ kicks directly from numerical relativity
Finding the shape of extremal black holes in beyond-GR theories
Just an update on talks I gave recently. Valeria Ferrari, Leonardo Gualtieri, and Paolo Pani hosted the conference “New Frontiers in Gravitational-Wave Astr...
Whenever you’ve got symmetry, you should use it!
One of the first numerical simulations of black hole mergers in beyond-GR effective field theories
My talk slides/movies from TG17 and APS17
My talk slides/movies from the EHT16 conference in Cambrige, MA
My talk slides/movies from the FF2016 conference at Northwestern
My talk slides/movies from the GR21 conference in NYC
I’m on Episode 64 of the Titanium Physicists Podcast
My talks slides/movies from the 2016 April APS meeting in SLC
Interactive tool for visualizing spherical/circular photon orbits in Kerr
I hosted a Quora session. It went well!
Invited review for CQG Focus Issue
I’m on Episode 62 of the Titanium Physicists Podcast
Progress in understanding the structure of extremal black holes in Chern-Simons
Interactive tool to compute Kerr quantities
Interactive tool to compute ISCOs in Kerr
A major review on non-GR theories, black holes and neutron stars in non-GR theories, compact binaries in non-GR theories, and pulsar, gravitational-wave, and...
Numerical solutions for rapidly-rotating dCS black holes show where the weak-coupling expansion breaks down.
MIT PhD thesis of Leo C. Stein
Interactive toy for understanding Poincaré sections and chaos
qnm is an open-source Python package for computing the Kerr quasinormal mode frequencies, angular separation constants, and spherical-spheroidal mixing coeff...
Accurate models of gravitational waves from merging black holes are necessary for detectors to observe as many events as possible while extracting the maximu...
Real-time interactive visualizations of merging black holes in seconds!
Modeling black holes remnants directly from numerical relativity
Modeling black holes’ kicks directly from numerical relativity
I’m releasing into the wild a simple code for computing neutron star structure in the slow-rotation expansion to first and second order. This code was origi...
Here to save you some algebra and column-inches
How to get remote jupyter to automatically open a local browser.
I just created a repo on github for computing complete elliptic integrals in javascript. The README.md is below, and a demo after that. You might ask yoursel...
If you’re in the intersection of git, emacs, and persnickety about whitespace.
That moment when social media creates scientific collaboration
I’m releasing into the wild a simple code for computing neutron star structure in the slow-rotation expansion to first and second order. This code was origi...
Not all theories with long-ranged scalar fields produce dipole radiation in binaries
A major review on non-GR theories, black holes and neutron stars in non-GR theories, compact binaries in non-GR theories, and pulsar, gravitational-wave, and...
Integrability conditions when trying to solve for a conformal factor
Interactive toy for understanding Poincaré sections and chaos
The dividing line between bound and plunging orbits is an algebraic variety
Interactive tool for visualizing spherical/circular photon orbits in Kerr
A generalization of symplectic integrators to non-conservative dynamics.
Extending Hamilton’s variational principle to nonconservative systems.
If you’re in the intersection of git, emacs, and persnickety about whitespace.
The dividing line between bound and plunging orbits is an algebraic variety
qnm is an open-source Python package for computing the Kerr quasinormal mode frequencies, angular separation constants, and spherical-spheroidal mixing coeff...
Hear me, Katie Bouman, and friends talk about how to snap a picture of a black hole with the Event Horizon Telescope!
A surrogate model extending the parameter space range of fully precessing quasicircular inspirals
Accurate models of gravitational waves from merging black holes are necessary for detectors to observe as many events as possible while extracting the maximu...
I’m on Episode 42 of the Starts with a Bang Podcast
Want to hear me talk about numerical relativity and theories beyond GR?
Real-time interactive visualizations of merging black holes in seconds!
Modeling black holes remnants directly from numerical relativity
Gravity theories beyond general relativity (GR) can change the properties of gravitational waves: their polarizations, dispersion, speed, and, importantly, e...
In theories of gravity that include a scalar field, a compact object’s scalar charge is a crucial quantity since it controls dipole radiation, which can be s...
Modeling black holes’ kicks directly from numerical relativity
Finding the shape of extremal black holes in beyond-GR theories
Whenever you’ve got symmetry, you should use it!
One of the first numerical simulations of black hole mergers in beyond-GR effective field theories
My talk slides/movies from the EHT16 conference in Cambrige, MA
I’m on Episode 64 of the Titanium Physicists Podcast
Interactive tool for visualizing spherical/circular photon orbits in Kerr
I hosted a Quora session. It went well!
Angular momentum is tricky to define in GR! Here’s an approach so that observers can all agree with each others’ measurements.
Invited review for CQG Focus Issue
I’m on Episode 62 of the Titanium Physicists Podcast
Not all theories with long-ranged scalar fields produce dipole radiation in binaries
Interactive tool to compute Kerr quantities
Interactive tool to compute ISCOs in Kerr
A major review on non-GR theories, black holes and neutron stars in non-GR theories, compact binaries in non-GR theories, and pulsar, gravitational-wave, and...
MIT PhD thesis of Leo C. Stein
Integrability conditions when trying to solve for a conformal factor
Here to save you some algebra and column-inches
An identity between vector commutation coefficients and coframe connection coefficients
These three objects form a superalgebra! Whoa!
When can you integrate-by-parts with Lie derivatives?
Special thanks to Ben Mares for coming up with this identity.
There is a nice 4-dimensional Weyl identity that I can never seem to remember off the top of my head; so I decided I need to write this note so I don’t have ...
The Weyl decomposition, further splitting into E/B, and computing in terms of 3+1 objects
In an effort to keep myself organized, I decided I should type up some notes I have laying around.
Angular momentum is tricky to define in GR! Here’s an approach so that observers can all agree with each others’ measurements.
If you’re in the intersection of git, emacs, and persnickety about whitespace.
The first astrophysically-relevant numerical simulation of merging black holes in a higher-curvature theory beyond GR.
qnm is an open-source Python package for computing the Kerr quasinormal mode frequencies, angular separation constants, and spherical-spheroidal mixing coeff...
The first numerical beyond-GR binary black hole merger simulation.
Gravity theories beyond general relativity (GR) can change the properties of gravitational waves: their polarizations, dispersion, speed, and, importantly, e...
One of the first numerical simulations of black hole mergers in beyond-GR effective field theories
I hosted a Quora session. It went well!
Not all theories with long-ranged scalar fields produce dipole radiation in binaries
A major review on non-GR theories, black holes and neutron stars in non-GR theories, compact binaries in non-GR theories, and pulsar, gravitational-wave, and...
The dividing line between bound and plunging orbits is an algebraic variety
The first astrophysically-relevant numerical simulation of merging black holes in a higher-curvature theory beyond GR.
qnm is an open-source Python package for computing the Kerr quasinormal mode frequencies, angular separation constants, and spherical-spheroidal mixing coeff...
The first numerical beyond-GR binary black hole merger simulation.
A surrogate model extending the parameter space range of fully precessing quasicircular inspirals
Accurate models of gravitational waves from merging black holes are necessary for detectors to observe as many events as possible while extracting the maximu...
Real-time interactive visualizations of merging black holes in seconds!
Modeling black holes remnants directly from numerical relativity
Gravity theories beyond general relativity (GR) can change the properties of gravitational waves: their polarizations, dispersion, speed, and, importantly, e...
In theories of gravity that include a scalar field, a compact object’s scalar charge is a crucial quantity since it controls dipole radiation, which can be s...
Modeling black holes’ kicks directly from numerical relativity
Finding the shape of extremal black holes in beyond-GR theories
Whenever you’ve got symmetry, you should use it!
One of the first numerical simulations of black hole mergers in beyond-GR effective field theories
MIT PhD thesis of Leo C. Stein
Finding the shape of extremal black holes in beyond-GR theories
Whenever you’ve got symmetry, you should use it!
Integrability conditions when trying to solve for a conformal factor
Interactive toy for understanding Poincaré sections and chaos
Real-time interactive visualizations of merging black holes in seconds!
Interactive toy for visualizing relationship between polynomial roots and coefficients
Interactive tool for visualizing spherical/circular photon orbits in Kerr
Interactive tool to compute Kerr quantities
Interactive tool to compute ISCOs in Kerr
How to get remote jupyter to automatically open a local browser.
How to get remote jupyter to automatically open a local browser.
I just created a repo on github for computing complete elliptic integrals in javascript. The README.md is below, and a demo after that. You might ask yoursel...
How to get remote jupyter to automatically open a local browser.
If you’re in the intersection of git, emacs, and persnickety about whitespace.
The first astrophysically-relevant numerical simulation of merging black holes in a higher-curvature theory beyond GR.
The first numerical beyond-GR binary black hole merger simulation.
A surrogate model extending the parameter space range of fully precessing quasicircular inspirals
Accurate models of gravitational waves from merging black holes are necessary for detectors to observe as many events as possible while extracting the maximu...
Want to hear me talk about numerical relativity and theories beyond GR?
Hear me, Katie Bouman, and friends talk about how to snap a picture of a black hole with the Event Horizon Telescope!
I’m on Episode 42 of the Starts with a Bang Podcast
Want to hear me talk about numerical relativity and theories beyond GR?
I’m on Episode 64 of the Titanium Physicists Podcast
I hosted a Quora session. It went well!
I’m on Episode 62 of the Titanium Physicists Podcast
qnm is an open-source Python package for computing the Kerr quasinormal mode frequencies, angular separation constants, and spherical-spheroidal mixing coeff...
Finding the shape of extremal black holes in beyond-GR theories
Whenever you’ve got symmetry, you should use it!
One of the first numerical simulations of black hole mergers in beyond-GR effective field theories
MIT PhD thesis of Leo C. Stein
Hear me, Katie Bouman, and friends talk about how to snap a picture of a black hole with the Event Horizon Telescope!
I’m on Episode 42 of the Starts with a Bang Podcast
I’m on Episode 64 of the Titanium Physicists Podcast
I’m on Episode 62 of the Titanium Physicists Podcast
Interactive toy for visualizing relationship between polynomial roots and coefficients
Not all theories with long-ranged scalar fields produce dipole radiation in binaries
A major review on non-GR theories, black holes and neutron stars in non-GR theories, compact binaries in non-GR theories, and pulsar, gravitational-wave, and...
qnm is an open-source Python package for computing the Kerr quasinormal mode frequencies, angular separation constants, and spherical-spheroidal mixing coeff...
Real-time interactive visualizations of merging black holes in seconds!
Modeling black holes remnants directly from numerical relativity
Modeling black holes’ kicks directly from numerical relativity
I missed the author index from LRR, so I rebuilt one.
How to get remote jupyter to automatically open a local browser.
I hosted a Quora session. It went well!
How to get remote jupyter to automatically open a local browser.
The first astrophysically-relevant numerical simulation of merging black holes in a higher-curvature theory beyond GR.
qnm is an open-source Python package for computing the Kerr quasinormal mode frequencies, angular separation constants, and spherical-spheroidal mixing coeff...
The first numerical beyond-GR binary black hole merger simulation.
Interactive toy for visualizing relationship between polynomial roots and coefficients
qnm is an open-source Python package for computing the Kerr quasinormal mode frequencies, angular separation constants, and spherical-spheroidal mixing coeff...
I’m releasing into the wild a simple code for computing neutron star structure in the slow-rotation expansion to first and second order. This code was origi...
How to get remote jupyter to automatically open a local browser.
I hosted a Quora session. It went well!
That moment when social media creates scientific collaboration
Sometimes in a numerical method, you need to be able to continuously turn a calculation on or off in space or time.
I just created a repo on github for computing complete elliptic integrals in javascript. The README.md is below, and a demo after that. You might ask yoursel...
How to get remote jupyter to automatically open a local browser.
Gravity theories beyond general relativity (GR) can change the properties of gravitational waves: their polarizations, dispersion, speed, and, importantly, e...
These three objects form a superalgebra! Whoa!
A surrogate model extending the parameter space range of fully precessing quasicircular inspirals
Modeling black holes remnants directly from numerical relativity
Modeling black holes’ kicks directly from numerical relativity
In theories of gravity that include a scalar field, a compact object’s scalar charge is a crucial quantity since it controls dipole radiation, which can be s...
Finding the shape of extremal black holes in beyond-GR theories
Whenever you’ve got symmetry, you should use it!
In theories of gravity that include a scalar field, a compact object’s scalar charge is a crucial quantity since it controls dipole radiation, which can be s...
How to get remote jupyter to automatically open a local browser.
That moment when social media creates scientific collaboration
Real-time interactive visualizations of merging black holes in seconds!
Want to hear me talk about numerical relativity and theories beyond GR?
Here to save you some algebra and column-inches
There is a nice 4-dimensional Weyl identity that I can never seem to remember off the top of my head; so I decided I need to write this note so I don’t have ...
I missed the author index from LRR, so I rebuilt one.