The cosmological collider in \(R^2\) inflation
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Publication:6585216
DOI10.1088/1475-7516/2024/07/010zbMATH Open1546.83232MaRDI QIDQ6585216
Publication date: 9 August 2024
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Cites Work
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- \(f(R)\) theories
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- <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
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- The Cosmological Optical Theorem
- Planck residuals anomaly as a fingerprint of alternative scenarios to inflation
- Classical cosmological collider physics and primordial features
- Continuous spectrum on cosmological collider
- Closed-form formulae for inflation correlators
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- Bootstrapping multi-field inflation: non-Gaussianities from light scalars revisited
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- Shapes of the cosmological low-speed collider
- Analytic formulae for inflationary correlators with dynamical mass
- A cosmological tachyon collider: enhancing the long-short scale coupling
- Cosmological collider signatures of Higgs-\(R^2\) inflation
- An effective cosmological collider
- Cosmological correlators with double massive exchanges: bootstrap equation and phenomenology
Related Items (3)
Fingerprints of a non-inflationary universe from massive fields ⋮ Cosmological correlators with double massive exchanges: bootstrap equation and phenomenology ⋮ Cosmological collider non-Gaussianity from multiple scalars and \(R^2\) gravity
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