Using Galaxy Evolution as Source of Physics-Based Ground Truth for Generative Models

Fuente: arXiv
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Autori principali: Li, Yun Qi, Do, Tuan, Jones, Evan, Boscoe, Bernie, Alfaro, Kevin, Nguyen, Zooey
Natura: Preprint
Pubblicazione: 2024
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author Li, Yun Qi
Do, Tuan
Jones, Evan
Boscoe, Bernie
Alfaro, Kevin
Nguyen, Zooey
author_facet Li, Yun Qi
Do, Tuan
Jones, Evan
Boscoe, Bernie
Alfaro, Kevin
Nguyen, Zooey
contents Generative models producing images have enormous potential to advance discoveries across scientific fields and require metrics capable of quantifying the high dimensional output. We propose that astrophysics data, such as galaxy images, can test generative models with additional physics-motivated ground truths in addition to human judgment. For example, galaxies in the Universe form and change over billions of years, following physical laws and relationships that are both easy to characterize and difficult to encode in generative models. We build a conditional denoising diffusion probabilistic model (DDPM) and a conditional variational autoencoder (CVAE) and test their ability to generate realistic galaxies conditioned on their redshifts (galaxy ages). This is one of the first studies to probe these generative models using physically motivated metrics. We find that both models produce comparable realistic galaxies based on human evaluation, but our physics-based metrics are better able to discern the strengths and weaknesses of the generative models. Overall, the DDPM model performs better than the CVAE on the majority of the physics-based metrics. Ultimately, if we can show that generative models can learn the physics of galaxy evolution, they have the potential to unlock new astrophysical discoveries.
format Preprint
id arxiv_https___arxiv_org_abs_2407_07229
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Using Galaxy Evolution as Source of Physics-Based Ground Truth for Generative Models
Li, Yun Qi
Do, Tuan
Jones, Evan
Boscoe, Bernie
Alfaro, Kevin
Nguyen, Zooey
Instrumentation and Methods for Astrophysics
Artificial Intelligence
Generative models producing images have enormous potential to advance discoveries across scientific fields and require metrics capable of quantifying the high dimensional output. We propose that astrophysics data, such as galaxy images, can test generative models with additional physics-motivated ground truths in addition to human judgment. For example, galaxies in the Universe form and change over billions of years, following physical laws and relationships that are both easy to characterize and difficult to encode in generative models. We build a conditional denoising diffusion probabilistic model (DDPM) and a conditional variational autoencoder (CVAE) and test their ability to generate realistic galaxies conditioned on their redshifts (galaxy ages). This is one of the first studies to probe these generative models using physically motivated metrics. We find that both models produce comparable realistic galaxies based on human evaluation, but our physics-based metrics are better able to discern the strengths and weaknesses of the generative models. Overall, the DDPM model performs better than the CVAE on the majority of the physics-based metrics. Ultimately, if we can show that generative models can learn the physics of galaxy evolution, they have the potential to unlock new astrophysical discoveries.
title Using Galaxy Evolution as Source of Physics-Based Ground Truth for Generative Models
topic Instrumentation and Methods for Astrophysics
Artificial Intelligence
url https://arxiv.org/abs/2407.07229