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Updated: Jul 24, 2025

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Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
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Dynamical Inflaton Coupled to Strongly Interacting Matter
Christian Ecker1, Elias Kiritsis2,3, Wilke van der Schee4,5
1Institut für Theoretische Physik, Goethe Universität, Max-von-Laue-Straße 1, 60438 Frankfurt am Main, Germany.
Physical Review Letters
|July 7, 2023
Summary
Cosmology
Area of Science:
- Cosmology
- Quantum Field Theory
- String Theory
Background:
- The inflationary theory explains particle creation during reheating after cosmic inflation.
- Understanding the universe's early stages requires reconciling gravity with quantum field theory.
Purpose of the Study:
- To self-consistently couple Einstein-inflaton equations with a holographic quantum field theory.
- To investigate the resulting cosmological evolution, including reheating and thermal equilibrium.
Main Methods:
- Coupling Einstein-inflaton equations to a strongly coupled quantum field theory via holography.
- Analyzing the theoretical framework to derive cosmological outcomes.
Main Results:
- Demonstrated a self-consistent model leading to an inflating universe.
- Showcased a reheating phase consistent with cosmological observations.
- Confirmed the emergence of a universe dominated by a thermalized quantum field theory.
Conclusions:
- The holographic approach provides a viable framework for understanding early universe cosmology.
- Reheating and thermal equilibrium are natural consequences of coupling gravity to strongly coupled quantum fields.
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