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Author (up) Dias, A.G.; Padovani, V.; Kannike, K.; Koivunen, N.; Leite, J.; Sanchez-Vega, B.L. url  doi
openurl 
  Title Dark matter in the scale-invariant 3-3-1-1 model Type Journal Article
  Year 2025 Publication Physical Review D Abbreviated Journal Phys. Rev. D  
  Volume 112 Issue 11 Pages 115017 - 19pp  
  Keywords  
  Abstract We propose a novel scale-invariant model with the 3-3-1-1 gauge symmetry featuring a universal seesaw mechanism for all fermion masses, which, through the inclusion of additional vectorlike quarks, provides a partial explanation for the observed fermion mass hierarchies. A discrete remnant of the gauge group, the matter parity (P-M), stabilizes a fermionic dark matter candidate, and the scalar sector includes two triplets (minimal for 3-3-1 breaking) and two scalar singlets. We identify the lightest P-M-odd fermion, f(d), as a viable dark matter candidate. Our analysis shows that f(d) satisfies the observed relic density constraint within the mass range 220 GeV less than or similar to mf(d) less than or similar to 555 GeV, primarily due to resonant annihilation via the new scalar H-2. While this mass range depends on the symmetry-breaking scale v(chi), which has a lower bound of v(chi) greater than or similar to 3.6 TeV from LEP constraints on the rho(0) parameter, we adopt a more conservative lower bound of v(chi) >10 TeV. This choice is made to ensure that the Z ' boson mass remains above approximately 4 TeV, and is motivated by recent LHC results and future projections for Z ' boson searches, which provide more stringent constraints than previous bounds or those from the rho(0) parameter. Spin-independent (SI) interactions dominate the direct detection phenomenology of f(d). We calculate the SI elastic scattering cross section and find that parameter points satisfying the relic density constraint are consistent with current experimental limits from LZ and PandaX-4T for certain parameter choices, particularly depending on the alpha(12) angle. Some regions of the viable parameter space lie below the neutrino floor. Prospects for detection by future experiments like XLZD and PandaX-xT are also presented and discussed.  
  Address [Dias, Alex G.; Padovani, Vinicius] Univ Fed ABC, Ctr Ciencias Nat Humanas, BR-09210580 Santo Andre, SP, Brazil, Email: vinicius.padovani.physics@gmail.com;  
  Corporate Author Thesis  
  Publisher Amer Physical Soc Place of Publication Editor  
  Language English Summary Language Original Title  
  Series Editor Series Title Abbreviated Series Title  
  Series Volume Series Issue Edition  
  ISSN 2470-0010 ISBN Medium  
  Area Expedition Conference  
  Notes WOS:001636045200003 Approved no  
  Is ISI yes International Collaboration yes  
  Call Number IFIC @ pastor @ Serial 7001  
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