arXiv subjects

A. Carrillo-Monteverde

Publications and source records attributed to A. Carrillo-Monteverde.

7 recordsLinked to original sources

arXiv2026

Photon and neutrino fluxes from spheroidal dwarf galaxies in a decaying DM model

In this work, we investigate a decaying dark matter scenario and its associated indirect detection signatures. The model consists of a scalar singlet with a lifetime exceeding the age of the Universe. Stability is ensured by a $Z_2$ symmetry imposed on the Lagrangian, allowing decay through a non-minimal gravitational coupling. The decay of dark matter produces Standard Model particles, which subsequently yield products such as gamma rays, neutrinos, and charged particles. We computed the gamma-ray and neutrino fluxes generated by this candidate in the Milky Way and in 14 dwarf spheroidal galaxies, as well as the corresponding expected number of events in selected experiments, using dedicated numerical tools. Results are presented for three benchmark masses and three coupling values consistent with cosmological constraints, showing that the predicted signals can be observable in specific regions of parameter space.

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arXiv2025

Dark Matter signals in solar neutrinos fluxes as probe of non-linear symmetry breaking

Dark matter (DM) particles gravitationally captured by the Sun can accumulate in its core and subsequently annihilate, producing neutrino fluxes that may be detectable on Earth. The intensity of these fluxes is highly sensitive to the properties of the underlying DM model, especially when the DM candidate is a scalar particle originating from spontaneous or non-linear symmetry breaking mechanisms. In this work, we explore the potential of solar neutrino fluxes to distinguish between the Standard Model extended by a scalar singlet and the non-linear Higgs portal scenarios in the context of a future DM discovery. We compute the expected neutrino fluxes within the regions of parameter space consistent with both relic density and current direct detection limits. Our results show that the non-linear model predicts neutrino fluxes that are systematically larger than those of the linear case, typically by at least one order of magnitude, and up to six orders of magnitude for DM masses around 1 TeV. These findings suggest that solar neutrino observations could provide a valuable probe to discriminate between these competing dark matter frameworks.

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arXiv2025

Effective textures from a $[SU(3)]^3$ flavored scalar sector

Current constraints on flavor-changing neutral currents (FCNCs) strongly indicate that any new physics emerging at the 1-10 TeV scale must adhere to the Minimal Flavor Violation (MFV) principle, where Yukawa couplings are the sole sources of flavor violation. In this work, we present a model inspired by a gauged $SU(3)$ flavor symmetry that dynamically generates leptonic Yukawa matrices through effective operators. The model incorporates a scalar sector with two sets of flavons, characterized by their vacuum expectation values (VEVs), which govern the suppression scale of the Yukawa couplings and the hierarchy of neutrino masses. By leveraging phenomenologically viable Yukawa textures, we derive restrictions on the flavon VEVs and demonstrate the compatibility of the model with experimental neutrino oscillation data. Furthermore, the model predicts at least one neutrino mass to be strongly suppressed, consistent with the normal mass ordering and experimental upper bounds. This framework provides a robust mechanism for dynamically generating neutrino masses and mixing while addressing key challenges in leptonic flavor physics, such as FCNC suppression and CP-violating phases.

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arXiv2023

Signatures of Dipolar Dark Matter on Indirect Detection

In this work we study the annihilation of fermionic dark matter, considering it as a neutral particle with non-vanishing magnetic ($M$) and electric ($D$) dipole moments. Effective cross section of the process $χ\overlineχ \rightarrow γγ$ is computed starting from a general form of the coupling $χ\overlineχ γ$ in the framework of an extension of the Standard Model. By taking into account the annihilation of dark matter pairs into mono-energetic photons, we found that for masses of $O(10^2)$ GeV, an electric dipole moment $\sim 10^{-16}\, \textrm{e cm}$ is required to satisfy the current relic density inferences. Additionally, in order to pin down models viable to describe the physics of dark matter in the early Universe, we also constrain our model according to recent measurements of the temperature anisotropies of the cosmic microwave background radiation, and report constraints to the electric and magnetic dipole moments for a range of masses within our model.

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arXiv2020

On the Universal Texture in the PA-2HDM for the V-SPIN case

In a Partially Aligned Two Higgs Doublet Model, where only is allowed flavor violation between third and second generation of fermions, we propose a mechanism to generate the second Yukawa matrix through a Unitary V-Spin flavor transformation on the mass matrix for quarks and leptons. Also we assume that this flavor transformation is universal, this is, we use the same parameters to generate Yukawa matrix elements in both sectors, reducing drastically the number of free parameters. As consequence we obtained a serie of relations between Yukawa matrix elements, that we called the Universality Constraint. Also, we obtained an interval of values for the second Yukawa matrix elements, expressed in terms of the Cheng and Sher ansatz, for $τ\to\ muμ^+μ^-$ and $τ\toγμ$ coming from the Universality Constraint and experimental bounds for light scalar masses. Finally, we show the allowed region of parameters for the flavor transformation from $B_s\toμμ$ decays, $B_s^0-\bar{B}_s^0$ mixing, $τ\toμμ^+μ^-$ and $τ\toγμ$ experimental bounds.

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arXiv2019

Phenomenology of the Partially Aligned 2HDM with leptonic decay of mesons

In this paper we present a phenomenological analysis of the Partially Aligned Two Higgs Doublet Model (PA-2HDM) by using leptonic decays of mesons and $B^0_{d,s}$-$\bar B^0_{d,s}$ mixing. We focus our attention in a scenario where the leading contribution to FCNC is given by the tree level interaction with the light pseudoscalar $A^0$ ($M_{A^0}\sim 250$ GeV). We show how an underlying flavor symmetry controls FCNC in the quark and lepton couplings with the pseudoscalar, without alignment between Yukawa matrices. Upper bounds on the free parameters are calculated in the context of the leptonic decays $B^0_{s,d}\toμ^+μ^-$ and $K^0_L\to μ^+μ^-$ and $B^0_{s,d}$ mixing. Also, our assumptions implies that bounds on New Physics contribution in the quark sector coming from $B^0_{s,d}$ mixing impose an upper bound on the parameters for the leptonic sector. Finally we give predictions of branching ratios for leptonic decay of mesons with FCNC and LFV.

hep-ph↗

arXiv2018

Dark Matter Direct Detection from new interactions in models with spin-two mediators

We consider models where a massive spin-two resonance acts as the mediator between Dark Matter (DM) and the SM particles through the energy-momentum tensor. We examine the effective theory for fermion, vector and scalar DM generated in these models and find novel types of DM-SM interaction never considered before. We identify the effective interactions between DM and the SM quarks when the mediator is integrated out, and match them to the gravitational form factors relevant for spin-independent DM-nucleon scattering. We also discuss the interplay between DM relic density conditions, direct detection bounds and collider searches for the spin-two mediator.

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