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Primordial Non-Gaussianities and Zero-Bias Tracers of the Large-Scale Structure
Emanuele Castorina1,2, Yu Feng1,2, Uroš Seljak1,2
1Berkeley Center for Cosmological Physics, University of California, Berkeley, California 94720, USA.
Physical Review Letters
|September 22, 2018
Summary
Researchers developed a new method to constrain primordial non-Gaussianities using unclustered tracers. This technique significantly improves precision, potentially reaching σ_{f_{NL}^{loc}}≃1 with high-density tracers.
Area of Science:
- Cosmology
- Large-Scale Structure Formation
- Statistical Analysis
Background:
- Primordial non-Gaussianities provide crucial insights into the early universe.
- Current methods for constraining local primordial non-Gaussianities (fNLloc) face limitations in precision.
- Large-scale structure (LSS) tracers are essential for probing cosmological parameters.
Purpose of the Study:
- To develop a novel method for constraining local primordial non-Gaussianities.
- To investigate the effectiveness of unclustered tracers for improving precision.
- To propose a practical technique for constructing optimal tracers.
Main Methods:
- Utilizing unclustered tracers of the large-scale structure.
- Developing a method to construct tracers using environmental information.
- Validating the technique with N-body simulations.
Main Results:
- Unclustered, zero-bias tracers offer significant improvements over standard methods.
- The primary advantage stems from the vanishing of sampling variance.
- The proposed method demonstrates the potential to reach σ_{f_{NL}^{loc}}≃1.
Conclusions:
- A new, effective method for constraining local primordial non-Gaussianities has been developed.
- Unclustered tracers are a powerful tool for enhancing precision in cosmological measurements.
- The technique is robust and validated by simulations, paving the way for future studies.
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