English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Zendy Open

Presents the pdf analysis as premium feature

PDF Analysis

Insights

Presents the summarisation as premium feature

Summarisation

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the zaia usage as premium feature

ZAIA

Zendy Tools

Zendy Plus

Presents the access of premium content as premium feature

Premium Content

In the presence of non-minimal gravitational coupling $ \xi H^\dagger H {\calR}$ between the standard model (SM) Higgs doublet $H$ and the curvature scalar${\cal R}$, the effective ultraviolet cutoff scale is given by $\Lambda_{\rmcut}\approx m_P/\xi$, where $m_P$ is the reduced Planck mass, and $\xi \gtrsim1$ is a dimensionless coupling constant. In type I and type III seesaw extendedSM, which can naturally explain the observed solar and atmospheric neutrinooscillations, we investigate the implications of this non-minimal gravitationalcoupling for the SM Higgs boson mass bounds based on vacuum stability andperturbativity arguments. A lower bound on the Higgs boson mass close to 120GeV is realized with type III seesaw and $\xi \sim 10-10^3$.

Higgs Boson Mass Bounds in Seesaw Extended Standard Model with Non-Minimal Gravitational Coupling