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J. M. Dávila

Publications and source records attributed to J. M. Dávila.

2 recordsLinked to original sources

Exploring correlations between HEFT Higgs couplings $κ_V$ and $κ_{2V}$ via HH production at $e^+e^-$ colliders

In this work we explore the phenomenological implications at future $e^+e^-$ colliders of assuming anomalous couplings of the Higgs boson to gauge bosons $HVV$ and $HHVV$ ($V=W,Z$) given by the $κ$-modifiers with respect to the Standard Model couplings, $κ_V$ and $κ_{2V}$, respectively. For this study we use the Higgs Effective Field Theory (HEFT) where these two $κ$ parameters are identified with the two most relevant effective couplings at leading order, concretely $a=κ_V$ and $b=κ_{2V}$. Our focus is put on these two couplings and their potential correlations which we believe carry interesting information on the underlying ultraviolet theory. The particular studied process is $e^+e^- \to HH ν\bar ν$, where the vector boson scattering subprocess $WW \to HH$ plays a central role, specially at the largest planned energy colliders. Our detailed study of this process as a function of the energy and the angular variables indicates that the produced Higgs bosons in the BSM scenarios will have in general a high transversality as compared to the SM case if $κ_V^2 \neq κ_{2V}$. In order to enhance the sensitivity to these HEFT parameters $κ_V$ and $κ_{2V}$ and their potential correlations we propose here some selected differential cross sections for the $e^+e^- \to HH ν\barν$ process where different kinematic properties of the BSM case with respect to the SM are manifested. Finally, we will focus on the dominant Higgs decays to $b \bar b$ pairs leading to final events with 4 $b$-jets and missing transverse energy from the undetected neutrinos and will provide the expected accessibility to the $(κ_V,κ_{2V})$ effective couplings and their potential correlations. In our study we will consider the three projected energies for $e^+e^-$ colliders of 500 GeV, 1000 GeV and 3000 GeV.

hep-ph↗

Observations of compact stars and fermion-boson stars with a quartic self-interaction

We investigated the possibility that compact stars could be described by a fermion-boson star with a quartic self-interaction in the boson sector. Specifically, by varying the polytropic constant $K$ and adiabatic index $Γ$ in the polytropic equation of state, the boson mass $μ$, and the self-interaction parameter $Λ$, we construct equilibrium configurations of these mixed-stars with total mass compatible with the mass constraints obtained from observational data of the collaborations NICE, NICER/XMN-Newton, and LIGO. Our work confirms that the addition of a boson sector eases the comparison of neutron star models with gravitational events related to compact objects and that in such a case observations may have preference for a positive self-interaction in the boson sector.

gr-qc↗