Dark clouds to silver linings over the hyperchargeless scalar triplets

Fuente: arXiv
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Autores principales: Bandyopadhyay, Priyotosh, Parashar, Snehashis
Formato: Preprint
Publicado: 2025
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author Bandyopadhyay, Priyotosh
Parashar, Snehashis
author_facet Bandyopadhyay, Priyotosh
Parashar, Snehashis
contents A real scalar triplet with zero hypercharge offers a minimal non-trivial extension of the Standard Model (SM) with a charged Higgs and a possible dark matter or custodial symmetry breaking signature. The $Z_2$-odd inert triplet model (ITM) provides a dark matter, while the non-inert Higgs triplet model (HTM) breaks the custodial symmetry, enabling rich collider signatures. Both these models also promise the viability of a first-order phase transition (FOPT). This letter revisits both models under various theoretical and current experimental constraints, revealing a trade-off between DM and FOPT viability, and explores the resulting gravitational wave signals and collider prospects.
format Preprint
id arxiv_https___arxiv_org_abs_2505_23257
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Dark clouds to silver linings over the hyperchargeless scalar triplets
Bandyopadhyay, Priyotosh
Parashar, Snehashis
High Energy Physics - Phenomenology
A real scalar triplet with zero hypercharge offers a minimal non-trivial extension of the Standard Model (SM) with a charged Higgs and a possible dark matter or custodial symmetry breaking signature. The $Z_2$-odd inert triplet model (ITM) provides a dark matter, while the non-inert Higgs triplet model (HTM) breaks the custodial symmetry, enabling rich collider signatures. Both these models also promise the viability of a first-order phase transition (FOPT). This letter revisits both models under various theoretical and current experimental constraints, revealing a trade-off between DM and FOPT viability, and explores the resulting gravitational wave signals and collider prospects.
title Dark clouds to silver linings over the hyperchargeless scalar triplets
topic High Energy Physics - Phenomenology
url https://arxiv.org/abs/2505.23257