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The dynamical generation of right-handed-neutrino (RHN) masses in the early Universe naturally entails the formation of cosmic strings that give rise to an observable signal in gravitational waves (GWs).
1904
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N. Seto, S. Kawamura, and T. Nakamura, Possibility of direct measurement of the acceleration of the universe using 0.1-Hz band laser interferometer gravitational wave antenna in space
2001
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C. J. A. P. Martins and E. P. S. Shellard, Extending the velocity dependent one scale string evolution model
2002
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2002
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K. Schmitz, New Sensitivity Curves for Gravitational-Wave Experiments
2002
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A. Pilaftsis and T. E. J. Underwood, Resonant leptogenesis
2004
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L. Boubekeur, T. Hambye, and G. Senjanovic, Low scale leptogenesis and soft supersymmetry breaking
2004
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2017
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2017
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C. Ringeval and T. Suyama, Stochastic gravitational waves from cosmic string loops in scaling
2017
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T. Han and X. Wang, Radiative Decays of the Higgs Boson to a Pair of Fermions
2017
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2018
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C. Caprini and D. G. Figueroa, Cosmological Backgrounds of Gravitational Waves
2018
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V. Domcke and K. Schmitz, Inflation from High-Scale Supersymmetry Breaking
2018
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N. Okada and O. Seto, Probing the seesaw scale with gravitational waves
2018
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2018
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T. Hugle, M. Platscher, and K. Schmitz, Low-Scale Leptogenesis in the Scotogenic Neutrino Mass Model
2018
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2018
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2018
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2018
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N. Christensen, Stochastic Gravitational Wave Backgrounds
2019
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2019
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2019
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I. Brivio and M. Trott, Examining the neutrino option
2019
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2019
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2019
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2019
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2019
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