Investigating the Dark Sector with New Liht and HiddenParticles

Authors

DOI:

https://doi.org/10.47456/Cad.Astro.v7nEspecial.53337

Keywords:

dark matter, beyond Standard Model physics, dark sectors, early Universe

Abstract

Despite its success, the Standard Model (SM) of particle physics remains incomplete, with the absence of a dark matter (DM) candidate being one of its primary gaps. The lack of evidence for new heavy particles has driven interest toward light, feebly interacting DM candidates, whose thermal production in the early Universe
requires a portal mediator. In this work, we propose a model where a vector mediator, originating from a U(1)Q gauge symmetry, connects the visible sector to inelastic dark matter (iDM) candidates. Unlike the standard
dark photon scenario, in which SM fermions do not carry direct charges under the new symmetry, we explore Q charges defined by combinations of baryonic and leptonic numbers. We demonstrate that this framework
can alter the relic abundance calculation and the experimental phenomenology. Consequently, such models can unlock new windows in the parameter space, expanding the possibilities for DM discovery beyond the constraints of the conventional model.

Author Biography

  • Ana Luisa Foguel, Federal University of Rio de Janeiro

    Ana Luisa Foguel (afoguel@usp.br) é física formada pela Universidade Federal do Rio de Janeiro (UFRJ). Entre 2016 e 2020, integrou a colaboração do experimento CONNIE. Realizou o mestrado na Universidade de São Paulo (USP), onde atualmente cursa o doutorado. Durante o doutorado, realizou um estágio de pesquisa de um ano no Instituto de Física Teórica (IFT), em Madrid. Seus interesses de pesquisa incluem matéria e setores escuros, Universo primordial, leptogênese e sinais astrofísicos e cosmológicos de física além do Modelo Padrão.

References

[1] N. Aghanim et al., Planck 2018 results. VI. Cosmological parameters, Astron. Astrophys. 641, A6 (2020), [Erratum: Astron. Astrophys. 652, C4 (2021)].

[2] G. Jungman, M. Kamionkowski e K. Griest, Supersymmetric dark matter, Phys. Rept. 267, 195 (1996).

[3] G. Arcadi, M. Dutra, P. Ghosh, M. Lindner, Y. Mambrini, M. Pierre, S. Profumo e F. S. Queiroz, The waning of the WIMP? A review of models, searches, and constraints, Eur. Phys. J. C 78 (3), 203 (2018).

[4] L. Roszkowski, E. M. Sessolo e S. Trojanowski, WIMP dark matter candidates and searches—current status and future prospects, Rept. Prog. Phys. 81 (6), 066201

[5] E. Izaguirre, G. Krnjaic e B. Shuve, Discovering Inelastic Thermal-Relic Dark Matter at Colliders, Phys. Rev. D 93 (6), 063523 (2016).

[6] E. Izaguirre, Y. Kahn, G. Krnjaic e M. Moschella, Testing Light Dark Matter Coannihilation With Fixed-Target Experiments, Phys. Rev. D 96 (5), 055007 (2017).

[7] M. Fabbrichesi, E. Gabrielli e G. Lanfranchi, The Dark Photon (2020).

[8] A. L. Foguel, P. Reimitz e R. Z. Funchal, Unlocking the inelastic Dark Matter window with vector mediators, JHEP 05, 001 (2025).

[9] G. Steigman, B. Dasgupta e J. F. Beacom, Precise Relic WIMP Abundance and its Impact on Searches for Dark Matter Annihilation, Phys. Rev. D 86, 023506 (2012).

[10] https://github.com/anafoguel/ReD-DeLiVeR.

[11] D. W. P. d. Amaral, D. G. Cerdeno, P. Foldenauer e E. Reid, Solar neutrino probes of the muon anomalous magnetic moment in the gauged U(1) L µ −L τ, JHEP 12, 155 (2020).

[12] S. Tulin, New weakly-coupled forces hidden in low-energy QCD, Phys. Rev. D 89 (11), 114008 (2014).

[13] B. Aubert et al., The BaBar detector, Nucl. Instrum. Meth. A 479, 1 (2002).

[14] J. Z. Bai et al., The BES upgrade, Nucl. Instrum. Meth. A 458, 627 (2001).

[15] W. Altmannshofer et al., The Belle II Physics Book, PTEP 2019 (12), 123C01 (2019), [Erratum: PTEP 2020, 029201 (2020)].

[16] M. Kirsanov, Recent results of the NA64 experiment at the CERN SPS, EPJ Web Conf. 212, 06005 (2019).

[17] J. D. Bjorken, S. Ecklund, W. R. Nelson, A. Abashian, C. Church, B. Lu, L. W. Mo, T. A. Nunamaker e P. Rassmann, Search for Neutral Metastable Penetrating Particles Produced in the SLAC Beam Dump, Phys. Rev. D 38, 3375 (1988).

[18] T. Åkesson et al., Light Dark Matter eXperiment (LDMX) (2018).

[19] J. Blumlein et al., Limits on neutral light scalar and pseudoscalar particles in a proton beam dump experiment, Z. Phys. C 51, 341 (1991).

[20] A. N. Diddens et al., A Detector for Neutral Current Interactions of High-energy Neutrinos, Nucl. Instrum. Meth. 178, 27 (1980).

[21] A. A. Aguilar-Arevalo et al., Dark Matter Search in a Proton Beam Dump with MiniBooNE, Phys. Rev. Lett. 118 (22), 221803 (2017).

[22] A. A. Aguilar-Arevalo et al., Dark Matter Search in Nucleon, Pion, and Electron Channels from a Proton Beam Dump with MiniBooNE, Phys. Rev. D 98 (11), 112004 (2018).

[23] L. B. Auerbach et al., Measurement of electron - neutrino - electron elastic scattering, Phys. Rev. D 63, 112001 (2001).

[24] E. Cortina Gil et al., The Beam and detector of the NA62 experiment at CERN, JINST 12 (05), P05025 (2017).

[25] A. M. Sirunyan et al., Search for an L µ − L τ gauge boson using Z → 4µ events in protonproton collisions at √s = 13 TeV, Phys. Lett. B 792, 345 (2019).

[26] H. Abreu et al., The FASER detector, JINST 19 (05), P05066 (2024).

[27] A. Ariga et al., FASER’s physics reach for long-lived particles, Phys. Rev. D 99 (9), 095011 (2019).

[28] J. L. Feng et al., The Forward Physics Facility at the High-Luminosity LHC, J. Phys. G 50 (3), 030501 (2023).

[29] R. Aaij et al., Search for Dark Photons Produced in 13 TeV pp Collisions, Phys. Rev. Lett. 120 (6), 061801 (2018).

[30] C. Giovanetti, M. Lisanti, H. Liu e J. T. Ruderman, Joint Cosmic Microwave Background and Big Bang Nucleosynthesis Constraints on Light Dark Sectors with Dark Radiation, Phys. Rev. Lett. 129 (2), 021302 (2022).

[31] A. Berlin, G. Krnjaic e E. Pinetti, Reviving MeV-GeV Indirect Detection with Inelastic Dark Matter (2023).

[32] D. K. Ghosh, P. Ghosh, S. Jeesun e R. Srivastava, The N eff at CMB challenges U(1) X light gauge boson scenarios (2024).

[33] L. Wolfenstein, Neutrino Oscillations in Matter, Phys. Rev. D 17, 2369 (1978).

[34] M. M. Guzzo, A. Masiero e S. T. Petcov, On the MSW effect with massless neutrinos and no mixing in the vacuum, Phys. Lett. B 260, 154 (1991).

[35] T. Han, J. Liao, H. Liu e D. Marfatia, Nonstandard neutrino interactions at COHERENT, DUNE, T2HK and LHC, JHEP 11, 028 (2019).

[36] P. Coloma, M. C. Gonzalez-Garcia e M. Maltoni, Neutrino oscillation constraints on U(1)’ models: from non-standard interactions to long-range forces, JHEP 01, 114 (2021), [Erratum: JHEP 11, 115 (2022)].

[37] J. A. Dror, R. Lasenby e M. Pospelov, New constraints on light vectors coupled to anomalous currents, Phys. Rev. Lett. 119 (14), 141803 (2017).

[38] J. A. Dror, R. Lasenby e M. Pospelov, Dark forces coupled to nonconserved currents, Phys. Rev. D 96 (7), 075036 (2017).

Published

2026-07-30

How to Cite

[1]
A. L. Foguel, “Investigating the Dark Sector with New Liht and HiddenParticles”, Cad. Astro., vol. 7, no. Especial, pp. 13–24, Jul. 2026, doi: 10.47456/Cad.Astro.v7nEspecial.53337.