A convolutional neural network for cosmic string detection in CMB temperature maps
Abstract
We present in detail the convolutional neural network used in our previous work to detect cosmic strings in cosmic microwave background (CMB) temperature anisotropy maps. By training this neural network on numerically generated CMB temperature maps, with and without cosmic strings, the network can produce prediction maps that locate the position of the cosmic strings and provide a probabilistic estimate of the value of the string tension Gμ. Supplying noiseless simulations of CMB maps with arcmin resolution to the network resulted in the accurate determination both of string locations and string tension for sky maps having strings with string tension as low as Gμ = 5 × 10-9, a result from our previous work. In this work we discuss the numerical details of the code that is publicly available online. Furthermore, we show that though we trained the network with a long straight string toy model, the network performs well with realistic Nambu-Goto simulations.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- May 2019
- DOI:
- 10.1093/mnras/stz491
- arXiv:
- arXiv:1708.08878
- Bibcode:
- 2019MNRAS.485.1377C
- Keywords:
-
- methods: data analysis;
- methods: statistical;
- techniques: image processing;
- cosmic background radiation;
- cosmology: theory;
- Astrophysics - Cosmology and Nongalactic Astrophysics;
- General Relativity and Quantum Cosmology;
- High Energy Physics - Phenomenology;
- High Energy Physics - Theory
- E-Print:
- 8 pages, 2 figures. v2 to 3: Introduction shortened and formatting adjustments to more closely match published version. v1 to v2: Cleaned up confusing notation and writing. Added more details and examples to clarify our presentation. Announced the public availability of the code online. Changed the formatting of the paper