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Massless spinning correlators in cosmology are extremely complicated. In contrast, the scattering amplitudes of massless particles with spin are very simple. We propose that the reason for the unreasonable complexity of these correlators lies in the
Externí odkaz:
http://arxiv.org/abs/2408.02727
The $\alpha'$-complete cosmology developed by Hohm and Zwiebach classifies the ${\rm O}(d,d;{\mathbb R})$ invariant theories involving metric, $b$-field and dilaton that only depend on time, to all orders in $\alpha'$. Some of these theories feature
Externí odkaz:
http://arxiv.org/abs/2011.10091
Akademický článek
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The $��'$-complete cosmology developed by Hohm and Zwiebach classifies the ${\rm O}(d,d;{\mathbb R})$ invariant theories involving metric, $b$-field and dilaton that only depend on time, to all orders in $��'$. Some of these theories feature
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::9bfcd5d57a0778d20b66b881db90ccd6
Publikováno v:
Journal of High Energy Physics; Mar2021, Vol. 2021 Issue 3, p1-42, 42p
