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We present a set of tools to assess the capabilities of LISA to detect and reconstruct the spectral shape and amplitude of a stochastic gravitational wave background (SGWB).
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P. Adshead, E. Martinec and M. Wyman, Perturbations in Chromo-Natural Inflation , JHEP 09
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V. Domcke, F. Muia, M. Pieroni and L. T. Witkowski, PBH dark matter from axion inflation , JCAP 1707
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O. Özsoy, On Synthetic Gravitational Waves from Multi-field Inflation , JCAP 1804
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P. Meyers, Cross-correlation searches for persistent gravitational waves with Advanced LIGO and noise studies for current and future ground-based gravitational-wave detectors , Ph.D. thesis, University of Minnesota, 2018
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M. Armano et al., Beyond the Required LISA Free-Fall Performance: New LISA Pathfinder Results down to 20 μ \mu Hz , Phys. Rev. Lett. 120
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A. Kosowsky, M. S. Turner and R. Watkins, Gravitational waves from first order cosmological phase transitions , Phys. Rev. Lett. 69
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