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Updated: May 3, 2026

Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
Testing the self-consistency of the excursion set approach to predicting the dark matter halo mass function
I Achitouv1, Y Rasera2, R K Sheth3
1Ludwig-Maximilians-Universitat München, Universitäts-Sternwarte München, Scheinerstrasse 1, D-81679 München, Germany and Excellence Cluster Universe, Boltzmannstrasse 2, D-85748 Garching bei München, Germany and Laboratoire Univers et Théories (LUTh), UMR 8102 CNRS, Observatoire de Paris, Université Paris Diderot, 5 Place Jules Janssen, 92190 Meudon, France.
The excursion set approach models dark matter halo abundance using a critical overdensity threshold. A drifting diffusing barrier model offers a self-consistent description of halo abundance and protohalo overdensities.
Area of Science:
- Cosmology
- Astrophysics
- Statistical Mechanics
Background:
- The excursion set approach is a theoretical framework for predicting dark matter halo abundance.
- A critical overdensity threshold (barrier) is essential for this formalism.
- The physical meaning of this barrier is unclear due to averaging over initial field positions.
Purpose of the Study:
- To investigate the physical motivation and meaning of the barrier in the excursion set approach.
- To develop a self-consistent model for halo abundance predictions.
Main Methods:
- Analyzing the statistical assumptions underlying the excursion set approach.
- Implementing a drifting diffusing barrier model.
Main Results:
- The drifting diffusing barrier model provides a self-consistent description of halo abundance.
- This model accurately describes the initial overdensities of protohalo patches.
Conclusions:
- The drifting diffusing barrier model offers a physically motivated and consistent description within the excursion set framework.
- This approach enhances the predictive power of dark matter halo formation models.
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