Fast and credible likelihood-free cosmology with truncated marginal neural ratio estimation
Alex Cole, B. Miller, Samuel J. Witte, Maxwell Xu Cai, Meiert W. Grootes, Francesco Nattino, Christoph Weniger
No strong AI-core implementation/artifact signals were detected from current providers.
Abstract Sampling-based inference techniques are central to modern cosmological data analysis; these methods, however, scale poorly with dimensionality and typically require approximate or intractable likelihoods. In this paper we describe how Truncated Marginal Neural Ratio Estimation ( tmnre ) (a new approach in so-called simulation-based inference) naturally evades these issues, improving the ( i ) efficiency, ( i ...
i ) scalability, and ( iii ) trustworthiness of the inference. Using measurements of the Cosmic Microwave Background (CMB), we show that tmnre can achieve converged posteriors using orders of magnitude fewer simulator calls than conventional Markov Chain Monte Carlo ( mcmc ) methods. Remarkably, in these examples the required number of samples is effectively independent of the number of nuisance parameters. In addition, a property called local amortization allows the performance of rigorous statistical consistency checks that are not accessible to sampling-based methods. tmnre promises to become a powerful tool for cosmological data analysis, particularly in the context of extended cosmologies, where the timescale required for conventional sampling-based inference methods to converge can greatly exceed that of simple cosmological models such as ΛCDM. To perform these computations, we use an implementation of tmnre via the open-source code swyft .[ swyft is available at https://github.com/undark-lab/swyft . Demonstration on cosmological simulators used in this paper is available at https://github.com/a-e-cole/swyft-CMB .]
Results & Benchmarks
No concrete benchmark grounding is available yet. Treat the page as context or an implementation starting point only.
Abstract Sampling-based inference techniques are central to modern cosmological data analysis; these methods, however, scale poorly with dimensionality and typically require approximate or intractable likelihoods.
Implementation Evidence Summary
Recommendation evidence is currently too limited for a maintained-repo choice. Use Implementation Status and Reproduction Path for a practical baseline plan.
Reproduction Risks
- Estimate is based on paper-only reproduction flow
Hardware Notes
Expect multi-day setup/compute for meaningful reproduction based on current guidance.
Evidence disclosure
Evidence graph: 2 refs, 1 links.
Utility signals: depth 65/100, grounding 58/100, status medium.
Implementation Status
There is no verified maintained implementation yet. Use this baseline plan to decide whether to prototype now or defer.
- No direct maintained implementation was found. Use the paper PDF and citation graph to design a baseline reproduction.
- Start from related paper: Future projects on the Cosmic Microwave Background.
- Track assumptions and missing details in an experiment log before coding.
Reproduction readiness
Hardware requirements
- Expect multi-day setup/compute for meaningful reproduction based on current guidance.
No verified implementation available
- · No maintained repository has been identified for this paper. Check adjacent implementations or HF artifacts below.
No benchmark numbers could be verified. You will not be able to validate reproduction correctness against published numbers.
Hugging Face artifacts
No trustworthy direct or curated related Hugging Face artifacts were found yet.
Continue with targeted Hugging Face searches derived from the paper title and method context:
Datasets
Tip: start with models, then check datasets/spaces if you need evaluation data or demos.
Direct artifact matches are currently sparse. Use targeted Hugging Face searches to quickly locate candidate models, datasets, and demos.
Research context
53
Citations
158
References
Tasks
Cosmic microwave background, Markov chain Monte Carlo, Cosmology, Inference, Sampling (signal processing), Scalability, Context (archaeology), Computer science
Methods
Algorithm
Domains
Physics, Statistical physics, Mathematics
Evaluation & Human Feedback Data
Open this paper in HFEPX to review benchmark signals, evaluation modes, and human-feedback protocol context.
Open in HFEPXExplore Similar Papers
Jump to Paper2Code search queries derived from this paper's research context.
Related papers
-
Search on Paper2Code
Future projects on the Cosmic Microwave Background (2008) Semantic similarity
-
Search on Paper2Code
Cosmological Parameter Estimation from CMB and X-ray clusters (2001) Semantic similarity
-
Search on Paper2Code
The Cosmic Microwave Background Spectrum (1997) Semantic similarity
-
Search on Paper2Code
Cosmological Parameter Estimation from CMB and X-ray clusters (2001) Semantic similarity
Need human evaluators for your AI research? Scale annotation with expert AI Trainers.