Cargando…

Semivisible dark photon phenomenology at the GeV scale

In rich dark sector models, dark photons heavier than tens of MeV can behave as semi-visible particles: their decays contain both visible and invisible final states. We present models containing multiple dark fermions which allow for such decays and inscribe them in the context of inelastic dark mat...

Descripción completa

Detalles Bibliográficos
Autores principales: Abdullahi, Asli M., Hostert, Matheus, Massaro, Daniele, Pascoli, Silvia
Lenguaje:eng
Publicado: 2023
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.108.015032
http://cds.cern.ch/record/2848795
_version_ 1780976864846675968
author Abdullahi, Asli M.
Hostert, Matheus
Massaro, Daniele
Pascoli, Silvia
author_facet Abdullahi, Asli M.
Hostert, Matheus
Massaro, Daniele
Pascoli, Silvia
author_sort Abdullahi, Asli M.
collection CERN
description In rich dark sector models, dark photons heavier than tens of MeV can behave as semi-visible particles: their decays contain both visible and invisible final states. We present models containing multiple dark fermions which allow for such decays and inscribe them in the context of inelastic dark matter and heavy neutral leptons scenarios. Our models represent a generalization of the traditional inelastic dark matter model by means of a charge conjugation symmetry. We revisit constraints on dark photons from $e^+e^-$ colliders and fixed target experiments, including the effect of analysis vetoes on semi-visible decays, $A^\prime \to \psi_i (\psi_j \to \psi_k \ell^+\ell^-)$. We find that in some cases, the BaBar and NA64 experiments no longer exclude large kinetic mixing, $\varepsilon \sim 10^{-2}$, and, specifically, the related explanation of the discrepancy in the muon $(g-2)$. This reopens an interesting window in parameter space for dark photons with exciting discovery prospects. We point out that a modified missing-energy search at NA64 can target short-lived $A^\prime$ decays and directly probe the newly-open parameter space.
id cern-2848795
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2023
record_format invenio
spelling cern-28487952023-10-02T04:38:24Zdoi:10.1103/PhysRevD.108.015032http://cds.cern.ch/record/2848795engAbdullahi, Asli M.Hostert, MatheusMassaro, DanielePascoli, SilviaSemivisible dark photon phenomenology at the GeV scalehep-exParticle Physics - Experimenthep-phParticle Physics - PhenomenologyIn rich dark sector models, dark photons heavier than tens of MeV can behave as semi-visible particles: their decays contain both visible and invisible final states. We present models containing multiple dark fermions which allow for such decays and inscribe them in the context of inelastic dark matter and heavy neutral leptons scenarios. Our models represent a generalization of the traditional inelastic dark matter model by means of a charge conjugation symmetry. We revisit constraints on dark photons from $e^+e^-$ colliders and fixed target experiments, including the effect of analysis vetoes on semi-visible decays, $A^\prime \to \psi_i (\psi_j \to \psi_k \ell^+\ell^-)$. We find that in some cases, the BaBar and NA64 experiments no longer exclude large kinetic mixing, $\varepsilon \sim 10^{-2}$, and, specifically, the related explanation of the discrepancy in the muon $(g-2)$. This reopens an interesting window in parameter space for dark photons with exciting discovery prospects. We point out that a modified missing-energy search at NA64 can target short-lived $A^\prime$ decays and directly probe the newly-open parameter space.In rich dark sector models, dark photons heavier than tens of MeV can behave as semivisible particles; their decays contain both visible and invisible final states. We present models containing multiple dark fermions which allow for such decays and inscribe them in the context of inelastic dark matter and heavy neutral leptons scenarios. Our models represent a generalization of the traditional inelastic dark matter model by means of a charge conjugation symmetry. We revisit constraints on dark photons from <math display="inline"><msup><mi>e</mi><mo>+</mo></msup><msup><mi>e</mi><mo>-</mo></msup></math> colliders and fixed-target experiments, including the effect of analysis vetoes on semivisible decays, <math display="inline"><msup><mi>A</mi><mo>′</mo></msup><mo stretchy="false">→</mo><msub><mi>ψ</mi><mi>i</mi></msub><mo stretchy="false">(</mo><msub><mi>ψ</mi><mi>j</mi></msub><mo stretchy="false">→</mo><msub><mi>ψ</mi><mi>k</mi></msub><msup><mo>ℓ</mo><mo>+</mo></msup><msup><mo>ℓ</mo><mo>-</mo></msup><mo stretchy="false">)</mo></math>. We find that in some cases the BABAR and NA64 experiments no longer exclude large kinetic mixing, <math display="inline"><mi>ε</mi><mo>∼</mo><msup><mn>10</mn><mrow><mo>-</mo><mn>2</mn></mrow></msup></math>, and, specifically, the related explanation of the discrepancy in the muon (<math display="inline"><mrow><mi>g</mi><mo>-</mo><mn>2</mn></mrow></math>). This reopens an interesting window in parameter space for dark photons with exciting discovery prospects. We point out that a modified missing-energy search at NA64 can target short-lived <math display="inline"><msup><mi>A</mi><mo>′</mo></msup></math> decays and directly probe the newly-open parameter space.arXiv:2302.05410CERN-TH-2023-019FERMILAB-PUB-23-054-TIRMP-CP3-23-08oai:cds.cern.ch:28487952023-02-10
spellingShingle hep-ex
Particle Physics - Experiment
hep-ph
Particle Physics - Phenomenology
Abdullahi, Asli M.
Hostert, Matheus
Massaro, Daniele
Pascoli, Silvia
Semivisible dark photon phenomenology at the GeV scale
title Semivisible dark photon phenomenology at the GeV scale
title_full Semivisible dark photon phenomenology at the GeV scale
title_fullStr Semivisible dark photon phenomenology at the GeV scale
title_full_unstemmed Semivisible dark photon phenomenology at the GeV scale
title_short Semivisible dark photon phenomenology at the GeV scale
title_sort semivisible dark photon phenomenology at the gev scale
topic hep-ex
Particle Physics - Experiment
hep-ph
Particle Physics - Phenomenology
url https://dx.doi.org/10.1103/PhysRevD.108.015032
http://cds.cern.ch/record/2848795
work_keys_str_mv AT abdullahiaslim semivisibledarkphotonphenomenologyatthegevscale
AT hostertmatheus semivisibledarkphotonphenomenologyatthegevscale
AT massarodaniele semivisibledarkphotonphenomenologyatthegevscale
AT pascolisilvia semivisibledarkphotonphenomenologyatthegevscale