Rupert Croft

Professor Carnegie Mellon University

  • Pittsburgh PA

Rupert Croft's research includes the structure of the universe, galaxy formation, and the measurement of cosmological parameters.

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Carnegie Mellon University

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Biography

Rupert Croft is a professor in the Physics Department at Carnegie Mellon University. His research interests include the large-scale structure of the universe, galaxy formation, and the measurement of cosmological parameters. Croft has a DPhil from Oxford University.

Areas of Expertise

Physical Chemistry (incl. Structural)
Organic Chemistry
Astronomical and Space Sciences
Atomic, Molecular, Nuclear, Particle and Plasma Physics
Quantum Physics

Media Appearances

Milky Way-like galaxies may have existed in the early universe

Phys.org  online

2015-08-05

Di Matteo and fellow CMU Physics Professor Rupert Croft have long been at the forefront of simulation cosmology, completing some of the largest simulations ever created. Their current simulation, called BlueTides, is 100 times larger than previous simulations. It was so large that it monopolized all of the National Science Foundation (NSF) supercomputer BlueWater's memory and almost 1 million CPUs in order to complete the simulation.

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Media

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Education

Oxford University

Ph.D.

Astrophysics

1995

Imperial College

B.Sc.

Physics

1991

Articles

Modeling quasar proximity zones in a realistic cosmological environment with a self-consistent light curve

Monthly Notices of the Royal Astronomical Society

2024

We study quasar proximity zones in a simulation that includes a self-consistent quasar formation model and realistic intergalactic medium (IGM) environments. The quasar host halo is 1013 M⊙ at z = 6, more massive than typical halos studied in previous work. Between 6 < z < 7.5, the quasar luminosity varies rapidly, with a mean magnitude of MUV, mean = −24.8 and the fluctuation reaching up to two orders of magnitude. Using this light curve to post-process the dense environment around the quasar, we find that the proximity zone size (Rp) ranges between 0.5 and 5 pMpc. We show that the light curve variability causes a similar degree of scatter in Rp as does the density fluctuation, both of which result in a standard deviation of ∼0.3 pMpc.

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AI-assisted super-resolution cosmological simulations III: time evolution

Monthly Notices of the Royal Astronomical Society

2024

In this work, we extend our recently developed super-resolution (SR) model for cosmological simulations to produce fully time-consistent evolving representations of the particle phase-space distribution. We employ a style-based constrained generative adversarial network (StyleGAN), where the changing cosmic time is an input style parameter to the network. The matter power spectrum and halo mass function agree well with results from high-resolution N-body simulations over the full trained redshift range (10 ≤ z ≤ 0). Furthermore, we assess the temporal consistency of our SR model by constructing halo merger trees.

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High-redshift supermassive black hole mergers in simulations with dynamical friction modelling

Monthly Notices of the Royal Astronomical Society

2024

In the near future, projects like Laser Interferometer Space Antenna (LISA) and pulsar timing arrays are expected to detect gravitational waves from mergers between supermassive black holes, and it is crucial to precisely model the underlying merger populations now to maximize what we can learn from this new data. Here, we characterize expected high-redshift (z > 2) black hole mergers using the very large volume Astrid cosmological simulation, which uses a range of seed masses to probe down to low-mass black holes (BHs), and directly incorporates dynamical friction so as to accurately model the dynamical processes that bring black holes to the galaxy centre where binary formation and coalescence will occur.

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