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Institute of Astronomy

 

Thu 16 Apr 11:00: CANCELLED: James Rogers

Next External Talks - Thu, 16/04/2026 - 06:55
CANCELLED: James Rogers

In person

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Wed 29 Apr 16:00: Descending into the Modular Bootstrap

Next External Talks - Wed, 15/04/2026 - 15:27
Descending into the Modular Bootstrap

The modular bootstrap has been a powerful tool for carving out the landscape of allowed two-dimensional conformal field theories (CFTs).  In this colloquium, I describe a complementary approach to standard modular bootstrap bounds: using modern machine learning strategies to actively search for CFT spectra that yield a valid torus partition function.  Using insights from statistical inference and a custom singular-value-based optimizer, I present evidence for an obstruction to finding CFTs with small central charge and large spectral gaps, and I speculate on what this might imply for the structure of the CFT landscape.  Along the way, I reflect on “centaur” approaches to theoretical physics, where human physicists and artificial intelligence collaborate to explore spaces of theories that would be difficult to navigate alone.

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Wed 29 Apr 16:00: Descending into the Modular Bootstrap

Next External Talks - Wed, 15/04/2026 - 15:26
Descending into the Modular Bootstrap

The modular bootstrap has been a powerful tool for carving out the landscape of allowed two-dimensional conformal field theories (CFTs).  In this colloquium, I describe a complementary approach to standard modular bootstrap bounds: using modern machine learning strategies to actively search for CFT spectra that yield a valid torus partition function.  Using insights from statistical inference and a custom singular-value-based optimizer, I present evidence for an obstruction to finding CFTs with small central charge and large spectral gaps, and I speculate on what this might imply for the structure of the CFT landscape.  Along the way, I reflect on “centaur” approaches to theoretical physics, where human physicists and artificial intelligence collaborate to explore spaces of theories that would be difficult to navigate alone.

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Categories: Talks

Wed 29 Apr 16:00: Descending into the Modular Bootstrap

Next External Talks - Wed, 15/04/2026 - 15:26
Descending into the Modular Bootstrap

The modular bootstrap has been a powerful tool for carving out the landscape of allowed two-dimensional conformal field theories (CFTs).  In this colloquium, I describe a complementary approach to standard modular bootstrap bounds: using modern machine learning strategies to actively search for CFT spectra that yield a valid torus partition function.  Using insights from statistical inference and a custom singular-value-based optimizer, I present evidence for an obstruction to finding CFTs with small central charge and large spectral gaps, and I speculate on what this might imply for the structure of the CFT landscape.  Along the way, I reflect on “centaur” approaches to theoretical physics, where human physicists and artificial intelligence collaborate to explore spaces of theories that would be difficult to navigate alone.

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Categories: Talks

Wed 29 Apr 16:00: Descending into the Modular Bootstrap

Next External Talks - Wed, 15/04/2026 - 15:26
Descending into the Modular Bootstrap

The modular bootstrap has been a powerful tool for carving out the landscape of allowed two-dimensional conformal field theories (CFTs).  In this colloquium, I describe a complementary approach to standard modular bootstrap bounds: using modern machine learning strategies to actively search for CFT spectra that yield a valid torus partition function.  Using insights from statistical inference and a custom singular-value-based optimizer, I present evidence for an obstruction to finding CFTs with small central charge and large spectral gaps, and I speculate on what this might imply for the structure of the CFT landscape.  Along the way, I reflect on “centaur” approaches to theoretical physics, where human physicists and artificial intelligence collaborate to explore spaces of theories that would be difficult to navigate alone.

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Tue 12 May 16:00: Strange New Worlds

Next Colloquia - Fri, 10/04/2026 - 12:58
Strange New Worlds

Super-Earths and sub-Neptunes are the most abundant exoplanets discovered in our galaxy to date. However, much of their nature and origin remains shrouded in mystery. Generally speaking, super-Earths and sub-Neptunes are thought to have formed  as one population with primordial hydrogen-dominated envelopes. However, most super-Earths lost their primordial atmospheres via thermally driven winds. In my talk, I will present new planet formation and evolution models that include the interplay between physics and chemistry and apply them to Earth, super-Earths and sub-Neptunes. I will show that magma ocean – atmosphere interactions expected in sub-Neptune exoplanets lead to signatures in their transmission spectra that are readily observable with JWST . In addition, hydrogen is efficiently sequestered into the interior, oxidizing iron and endogenously producing water. I will conclude by discussing possible parallels between Earth’s formation and that of super-Earths, shedding new light on Earth’s primary water reservoir, origin of the light elements in its iron core and oxidation state.

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Tue 12 May 16:00: Strange New Worlds

Next Colloquia - Fri, 10/04/2026 - 12:38
Strange New Worlds

Abstract not available

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Fri 10 Apr 16:00: Test

Next Colloquia - Fri, 10/04/2026 - 11:52
Test

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Tue 05 May 13:00: Title to be confirmed

Next External Talks - Thu, 02/04/2026 - 12:57
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Mon 15 Jun 13:00: Title to be confirmed

Next External Talks - Fri, 27/03/2026 - 10:50
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Mon 08 Jun 13:00: Title to be confirmed

Next External Talks - Fri, 27/03/2026 - 10:49
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Mon 01 Jun 13:00: Title to be confirmed

Next External Talks - Fri, 27/03/2026 - 10:48
Title to be confirmed

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Tue 26 May 13:00: Title to be confirmed

Next External Talks - Fri, 27/03/2026 - 10:47
Title to be confirmed

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Mon 18 May 13:00: Title to be confirmed

Next External Talks - Fri, 27/03/2026 - 10:44
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Tue 12 May 13:00: Title to be confirmed

Next External Talks - Fri, 27/03/2026 - 10:42
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Tue 05 May 13:00: Title to be confirmed

Next External Talks - Fri, 27/03/2026 - 10:40
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Mon 27 Apr 13:00: Title to be confirmed

Next External Talks - Fri, 27/03/2026 - 10:39
Title to be confirmed

Abstract not available

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Thu 19 Mar 16:00: Descending into the Modular Bootstrap

Next External Talks - Thu, 19/03/2026 - 09:12
Descending into the Modular Bootstrap

The modular bootstrap has been a powerful tool for carving out the landscape of allowed two-dimensional conformal field theories (CFTs).  In this colloquium, I describe a complementary approach to standard modular bootstrap bounds: using modern machine learning strategies to actively search for CFT spectra that yield a valid torus partition function.  Using insights from statistical inference and a custom singular-value-based optimizer, I present evidence for an obstruction to finding CFTs with small central charge and large spectral gaps, and I speculate on what this might imply for the structure of the CFT landscape.  Along the way, I reflect on “centaur” approaches to theoretical physics, where human physicists and artificial intelligence collaborate to explore spaces of theories that would be difficult to navigate alone.

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Wed 18 Mar 14:00: From Protostars to Protoplanets: Towards a Population-level simulation study of gravitationally unstable gas discs

Next External Talks - Wed, 18/03/2026 - 12:31
From Protostars to Protoplanets: Towards a Population-level simulation study of gravitationally unstable gas discs

Simulations of collapsing giant molecular clouds show protostars forming with discs that may be massive enough to become gravitationally unstable. This may play a key role both in the formation of the star itself, and in the formation of giant planets through disc fragmentation. We extract a set of young discs (less than 1e5 years) from a global cloud collapse simulation (Bate 2012). We upscale the resolution of these discs using a novel particle splitting method and employ an improved radiative cooling approximation in our runs – both as a requirement to accurately capture fragmenting planetary-mass clumps. This suite of physically-motivated simulations from non-idealised initial conditions should provide a valuable insight into the frequency of disc fragmentation and any resultant protoplanetary population. In this talk I will present the workflow and numerical methods involved in this population study, as well as some key insights from early results

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