Chiral gravitational waves and baryon superfluid dark matter
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Publication:5023738
DOI10.1088/1475-7516/2018/05/003OpenAlexW2784927723WikidataQ129884963 ScholiaQ129884963MaRDI QIDQ5023738
Stephon H. S. Alexander, David Spergel, Evan McDonough
Publication date: 24 January 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1801.07255
Related Items (13)
Dynamical friction in superfluids ⋮ Physics beyond the Standard Model with circular polarization in the CMB and CMB-21cm cross-correlation ⋮ Baryon-Interacting Dark Matter: heating dark matter and the emergence of galaxy scaling relations ⋮ Growth of linear perturbations in a universe with superfluid dark matter ⋮ A critique of covariant emergent gravity ⋮ Inflation and electroweak symmetry breaking ⋮ Early dark energy in type IIB string theory ⋮ Primordial circular polarization in the cosmic microwave background ⋮ New scalar field quartessence ⋮ The equation of state of dark matter superfluids ⋮ Observable chiral gravitational waves from inflation in string theory ⋮ Vortices and waves in light dark matter ⋮ Unified superfluid dark sector
Cites Work
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- Axion inflation with an \(SU(2)\) gauge field: detectable chiral gravity waves
- Dark matter self-interactions and small scale structure
- Parametric resonance of entropy perturbations in massless preheating
- Review of strongly-coupled composite dark matter models and lattice simulations
- New Post-Newtonian Parameter to Test Chern-Simons Gravity
- Gravitationally bound BCS state as dark matter
- Asymmetric dark matter and baryogenesis from pseudoscalar inflation
- Physical Foundations of Cosmology
- Generating luminous and dark matter during inflation
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