Galaxy shape statistics in the effective field theory

DOI10.1088/1475-7516/2021/05/061zbMath1485.85021arXiv2012.04114OpenAlexW3165392709MaRDI QIDQ5028149

Nora Elisa Chisari, Zvonimir Vlah, Fabian Schmidt

Publication date: 8 February 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2012.04114

zbMATH Keywords

power spectrumgravitational lensingweak gravitational lensinggalaxy surveys

Mathematics Subject Classification ID

Diffraction, scattering (78A45) Perturbative methods of renormalization applied to problems in quantum field theory (81T15) Quantum field theory on curved space or space-time backgrounds (81T20) Galactic and stellar structure (85A15) Effective quantum field theories (81T12)

Related Items (2)

Lagrangian approach to super-sample effects on biased tracers at field level: galaxy density fields and intrinsic alignments ⋮ Quadratic shape biases in three-dimensional halo intrinsic alignments

Cites Work

• Weak gravitational lensing
• Large-scale galaxy bias
• An EFT description of galaxy intrinsic alignments
• Primordial gravitational waves from galaxy intrinsic alignments

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