Dark Matter Subhalos, Strong Lensing and Machine Learning
arXiv:2005.05353
Abstract
We investigate the possibility of applying machine learning techniques to images of strongly lensed galaxies to detect a low mass cut-off in the spectrum of dark matter sub-halos within the lens system. We generate lensed images of systems containing substructure in seven different categories corresponding to lower mass cut-offs ranging from down to . We use convolutional neural networks to perform a multi-classification sorting of these images and see that the algorithm is able to correctly identify the lower mass cut-off within an order of magnitude to better than 93% accuracy.
20 pages
References in corpus (57)
- TensorFlow: Large-Scale Machine Learning on Heterogeneous Distributed Systems
- ADADELTA: An Adaptive Learning Rate Method
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample
- Machine learning and the physical sciences
- The Aquarius Project: the subhalos of galactic halos
- Dark Matter Search Results from a One TonneYear Exposure of XENON1T
- Cold and Fuzzy Dark Matter
- Ultralight scalars as cosmological dark matter
- Results from a search for dark matter in the complete LUX exposure
- Small-Scale Challenges to the CDM Paradigm
- Sterile Neutrinos as Dark Matter
- Dark Matter Self-interactions and Small Scale Structure
- Cosmological Simulations with Self-Interacting Dark Matter I: Constant Density Cores and Substructure
- The Milky Way's bright satellites as an apparent failure of LCDM
- Earth-mass dark-matter haloes as the first structures in the early Universe
- Compound gravitational lensing as a probe of dark matter substructure within galaxy halos
- Lenstronomy: multi-purpose gravitational lens modelling software package
- Bayesian Strong Gravitational-Lens Modeling on Adaptive Grids: Objective Detection of Mass Substructure in Galaxies
- Fast Automated Analysis of Strong Gravitational Lenses with Convolutional Neural Networks
- The accretion history of dark matter halos III: A physical model for the concentration-mass relation
- Dark matter heats up in dwarf galaxies
- Possible dark matter annihilation signal in the AMS-02 antiproton data
- SHARP -- VII. New constraints on the dark matter free-streaming properties and substructure abundance from gravitationally lensed quasars
- The chosen few: the low mass halos that host faint galaxies
- Search for dijet resonances in proton-proton collisions at sqrt(s) = 13 TeV and constraints on dark matter and other models
- Uncertainties in Parameters Estimated with Neural Networks: Application to Strong Gravitational Lensing
- Linear perturbation theory for tidal streams and the small-scale CDM power spectrum
- The Substructure Hierarchy in Dark Matter Haloes
- Lensing substructure quantification in RXJ1131-1231: A 2 keV lower bound on dark matter thermal relic mass
- The impact of baryonic physics on the subhalo mass function and implications for gravitational lensing
- Measuring the power spectrum of dark matter substructure using strong gravitational lensing
- The core-cusp problem: a matter of perspective
- Substructure of fuzzy dark matter haloes
- Constraints on mediator-based dark matter and scalar dark energy models using TeV collision data collected by the ATLAS detector
- On the dark matter profile in Sculptor: Breaking the degeneracy with Virial shape parameters
- Deep Convolutional Neural Networks as strong gravitational lens detectors
- Evidence of a population of dark subhalos from Gaia and Pan-STARRS observations of the GD-1 stream
- Abundance matching with the mean star formation rate: there is no missing satellites problem in the Milky Way above
- Identifying Strong Lenses with Unsupervised Machine Learning using Convolutional Autoencoder
- Mining for Dark Matter Substructure: Inferring subhalo population properties from strong lenses with machine learning
- MeV Dark Matter and Small Scale Structure
- A Search for Dark Matter Annihilation in Galaxy Groups
- Using Convolutional Neural Networks to identify Gravitational Lenses in Astronomical images
- To beta or not to beta: can higher-order Jeans analysis break the mass-anisotropy degeneracy in simulated dwarfs?
- On the Power Spectrum of Dark Matter Substructure in Strong Gravitational Lenses
- Gravitational Lensing and the Power Spectrum of Dark Matter Substructure: Insights from the ETHOS N-body Simulations
- A Search for Dark Matter Annihilation in the Milky Way Halo
- A Dark Census: Statistically Detecting the Satellite Populations of Distant Galaxies
- Direct Detection of Dark Matter Substructure in Strong Lens Images with Convolutional Neural Networks
- Probing the small-scale structure in strongly lensed systems via transdimensional inference
- Differentiable Strong Lensing: Uniting Gravity and Neural Nets through Differentiable Probabilistic Programming
- Predicting dark matter halo formation in N-body simulations with deep regression networks
- Analyzing interferometric observations of strong gravitational lenses with recurrent and convolutional neural networks
- Quantifying the power spectrum of small-scale structure in semi-analytic galaxies
- Gravitational Imaging of CDM Substructure
- Hunt for dark subhalos in the galactic stellar field using computer vision
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