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Speaker: Rome Samanta (SSM)
Abstract: I will begin with a brief overview of topological defects, such as domain walls and cosmic strings, and their connection to the stochastic gravitational-wave background. I will review current developments in the literature and highlight the main theoretical and phenomenological directions being explored. I will then focus on two key aspects of these defects. First, I will discuss how topological-defect physics can be used as a probe of previously unexplored regimes in particle-physics models. Second, I will introduce a non-standard class of defects that we are currently developing and discuss their potential implications for pulsar timing array observations.
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