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Machine Studying Pins Down Cosmological Parameters

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• Physics 15, s111

Cosmological constraints will be improved by making use of machine studying to a mixture of knowledge from two main probes of the large-scale construction of the Universe.

T. Kacprzak and J. Fluri [1]

The historical past of the Universe is ruled by a handful of cosmological parameters, such because the present-day matter density and amplitude of density fluctuations ( Ωm and 𝜎8, respectively). Astronomers have measured these parameters by observing the large-scale construction of the Universe, however the measurement precision has been restricted by a number of parameter degeneracies. For instance, a rise in Ωm can counteract a lower in 𝜎8 and vice versa. Now Tomasz Kacprzak and Janis Fluri on the Swiss Federal Institute of Expertise (ETH), Zurich, have discovered a strategy to break such degeneracies, strengthening the constraints on these parameters [1].

The Universe’s large-scale construction is often probed by learning galaxy clustering or through a statistical gravitational-lensing signature known as weak gravitational lensing (see Viewpoint: Weak Lensing Turns into a Excessive-Precision Survey Science). Every of those methods has related parameter degeneracies: for galaxy clustering, Ωm and 𝜎8 can tackle any variety of values relying on the assumed galaxy bias, which quantifies how nicely seen matter traces invisible darkish matter; for weak lensing, Ωm and 𝜎8 are equally degenerate with the intrinsic alignment amplitude, which measures the extent to which galaxies are aligned with each other.

Kacprzak and Fluri discovered that these degeneracies may very well be lifted through the use of deep studying—a kind of machine studying impressed by the human mind—to carry out a collective evaluation of galaxy-clustering and weak-lensing knowledge. The researchers present that, for future large-scale-structure surveys, this method might tighten constraints on the galaxy bias and on the intrinsic alignment amplitude by elements of about 1.5 and eight, respectively. In flip, the tactic might considerably strengthen constraints on each Ωm and 𝜎8. Nonetheless, the group says that an improved knowledge evaluation and understanding of survey systematic results is required earlier than the method can be utilized in observe.

–Ryan Wilkinson

Ryan Wilkinson is a contract science editor and author based mostly in Durham, UK.

References

  1. T. Kacprzak and J. Fluri, “DeepLSS: Breaking parameter degeneracies in large-scale construction with deep-learning evaluation of mixed probes,” Phys. Rev. X 12, 031029 (2022).

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