Inferring dark matter substructure with astrometric lensing beyond the
power spectrum
- URL: http://arxiv.org/abs/2110.01620v1
- Date: Mon, 4 Oct 2021 18:00:00 GMT
- Title: Inferring dark matter substructure with astrometric lensing beyond the
power spectrum
- Authors: Siddharth Mishra-Sharma
- Abstract summary: We introduce a novel method to search for global dark matter-induced gravitational lensing signatures in astrometric datasets.
Our method based on neural likelihood-ratio estimation shows significantly enhanced sensitivity to a cold dark matter population.
- Score: 0.0
- License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
- Abstract: Astrometry -- the precise measurement of positions and motions of celestial
objects -- has emerged as a promising avenue for characterizing the dark matter
population in our Galaxy. By leveraging recent advances in simulation-based
inference and neural network architectures, we introduce a novel method to
search for global dark matter-induced gravitational lensing signatures in
astrometric datasets. Our method based on neural likelihood-ratio estimation
shows significantly enhanced sensitivity to a cold dark matter population and
more favorable scaling with measurement noise compared to existing approaches
based on two-point correlation statistics, establishing machine learning as a
powerful tool for characterizing dark matter using astrometric data.
Related papers
- A method based on Generative Adversarial Networks for disentangling physical and chemical properties of stars in astronomical spectra [0.16385815610837165]
In this work, an encoder-decoder architecture has been designed, where adversarial training is used in the context of astrophysical spectral analysis.
A scheme of deep learning is used with the aim of unraveling in the latent space the desired parameters of the rest of the information contained in the data.
To test the effectiveness of the method, synthetic astronomical data are used from the APOGEE and Gaia surveys.
arXiv Detail & Related papers (2024-11-08T20:45:09Z) - Real-time gravitational-wave inference for binary neutron stars using machine learning [71.29593576787549]
We present a machine learning framework that performs complete BNS inference in just one second without making any approximations.
Our approach enhances multi-messenger observations by providing (i) accurate localization even before the merger; (ii) improved localization precision by $sim30%$ compared to approximate low-latency methods; and (iii) detailed information on luminosity distance, inclination, and masses.
arXiv Detail & Related papers (2024-07-12T18:00:02Z) - Cosmology from Galaxy Redshift Surveys with PointNet [65.89809800010927]
In cosmology, galaxy redshift surveys resemble such a permutation invariant collection of positions in space.
We employ a textitPointNet-like neural network to regress the values of the cosmological parameters directly from point cloud data.
Our implementation of PointNets can analyse inputs of $mathcalO(104) - mathcalO(105)$ galaxies at a time, which improves upon earlier work for this application by roughly two orders of magnitude.
arXiv Detail & Related papers (2022-11-22T15:35:05Z) - Toward deep-learning-assisted spectrally-resolved imaging of magnetic
noise [52.77024349608834]
We implement a deep neural network to efficiently reconstruct the spectral density of the underlying fluctuating magnetic field.
These results create opportunities for the application of machine-learning methods to color-center-based nanoscale sensing and imaging.
arXiv Detail & Related papers (2022-08-01T19:18:26Z) - Inferring Structural Parameters of Low-Surface-Brightness-Galaxies with
Uncertainty Quantification using Bayesian Neural Networks [70.80563014913676]
We show that a Bayesian Neural Network (BNN) can be used for the inference, with uncertainty, of such parameters from simulated low-surface-brightness galaxy images.
Compared to traditional profile-fitting methods, we show that the uncertainties obtained using BNNs are comparable in magnitude, well-calibrated, and the point estimates of the parameters are closer to the true values.
arXiv Detail & Related papers (2022-07-07T17:55:26Z) - Supernova Light Curves Approximation based on Neural Network Models [53.180678723280145]
Photometric data-driven classification of supernovae becomes a challenge due to the appearance of real-time processing of big data in astronomy.
Recent studies have demonstrated the superior quality of solutions based on various machine learning models.
We study the application of multilayer perceptron (MLP), bayesian neural network (BNN), and normalizing flows (NF) to approximate observations for a single light curve.
arXiv Detail & Related papers (2022-06-27T13:46:51Z) - Deep Learning Models of the Discrete Component of the Galactic
Interstellar Gamma-Ray Emission [61.26321023273399]
A significant point-like component from the small scale (or discrete) structure in the H2 interstellar gas might be present in the Fermi-LAT data.
We show that deep learning may be effectively employed to model the gamma-ray emission traced by these rare H2 proxies within statistical significance in data-rich regions.
arXiv Detail & Related papers (2022-06-06T18:00:07Z) - alpha-Deep Probabilistic Inference (alpha-DPI): efficient uncertainty
quantification from exoplanet astrometry to black hole feature extraction [7.5042943749402555]
Inference is crucial in modern astronomical research, where hidden astrophysical features are estimated from indirect and noisy measurements.
Traditional approaches for posterior estimation include sampling-based methods and variational inference.
We propose alpha-DPI, a deep learning framework that learns an approximate posterior using alpha-divergence variational inference paired with a generative neural network.
arXiv Detail & Related papers (2022-01-21T00:58:10Z) - Constraining dark matter annihilation with cosmic ray antiprotons using
neural networks [0.0]
We present a new method that significantly accelerates simulations of secondary and dark matter Galactic cosmic ray antiprotons.
We identify importance sampling as particularly suitable for ensuring that the network is only evaluated in well-trained parameter regions.
The fully trained networks are released as DarkRayNet together with this work and achieve a speed-up of the runtime by at least two orders of magnitude compared to conventional approaches.
arXiv Detail & Related papers (2021-07-26T18:00:04Z) - Semi-parametric $\gamma$-ray modeling with Gaussian processes and
variational inference [9.405199445496429]
Mismodeling the uncertain, diffuse emission of Galactic origin can seriously bias the characterization of astrophysical gamma-ray data.
We introduce a novel class of methods that use Gaussian processes and variational inference to build flexible background and signal models for gamma-ray analyses.
arXiv Detail & Related papers (2020-10-20T17:04:37Z)
This list is automatically generated from the titles and abstracts of the papers in this site.
This site does not guarantee the quality of this site (including all information) and is not responsible for any consequences.