Model-independent constraints with extended dark matter EFT

被引:0
|
作者
Tommi Alanne
Giorgio Arcadi
Florian Goertz
Valentin Tenorth
Stefan Vogl
机构
[1] Max-Planck-Institut für Kernphysik,
[2] Dipartimento di Matematica e Fisica,undefined
[3] INFN — Sezione Roma Tre,undefined
[4] Max-Planck-Institut für Physik,undefined
关键词
Beyond Standard Model; Cosmology of Theories beyond the SM;
D O I
暂无
中图分类号
学科分类号
摘要
We systematically explore the phenomenology of the recently proposed extended dark matter effective field theory (eDMeft), which allows for a consistent effective description of DM scenarios across different energy scales. The framework remains applicable at collider energies and is capable of reproducing the correct relic abundance by including a dynamical mediator particle to the dark sector, while maintaining correlations dictated by gauge invariance in a ‘model-independent’ way. Taking into account present and future constraints from direct- and indirect-detection experiments, from collider searches for missing energy and for scalar resonances in vector-boson, di-jet, and Higgs-pair final states, as well as from the relic abundance as measured by Planck, we determine viable regions in the parameter space, both for scalar and pseudoscalar mediator. In particular, we point out regions where cancellations in the direct-detection cross section appear leading to allowed islands for scalar mediators that could be missed in a naive simplified-model approach, but are present in the full D = 5 effective theory, as well as a general opening of the parameter space due to consistently considering all operators at a given mass dimension. Thus, canonical WIMP-like scenarios can survive even the next generation of direct-detection experiments in different mass regimes, while potentially becoming testable at the high-luminosity LHC.
引用
收藏
相关论文
共 50 条
  • [41] Model-independent superhedging under portfolio constraints
    Arash Fahim
    Yu-Jui Huang
    Finance and Stochastics, 2016, 20 : 51 - 81
  • [42] MODEL-INDEPENDENT GLOBAL CONSTRAINTS ON NEW PHYSICS
    BURGESS, CP
    GODFREY, S
    KONIG, H
    LONDON, D
    MAKSYMYK, I
    PHYSICAL REVIEW D, 1994, 49 (11): : 6115 - 6147
  • [43] Model-independent constraints on the cosmological anisotropic stress
    Amendola, Luca
    Fogli, Simone
    Guarnizo, Alejandro
    Kunz, Martin
    Vollmer, Adrian
    PHYSICAL REVIEW D, 2014, 89 (06):
  • [44] Model-independent superhedging under portfolio constraints
    Fahim, Arash
    Huang, Yu-Jui
    FINANCE AND STOCHASTICS, 2016, 20 (01) : 51 - 81
  • [45] Model independent analysis of MeV scale dark matter: Cosmological constraints
    Choudhury, Debajyoti
    Sachdeva, Divya
    PHYSICAL REVIEW D, 2019, 100 (03)
  • [46] A model-independent determination of the expansion and acceleration rates of the universe as a function of redshift and constraints on dark energy
    Daly, RA
    Djorgovski, SG
    ASTROPHYSICAL JOURNAL, 2003, 597 (01): : 9 - 20
  • [47] Model-independent distance measurements from gamma-ray bursts and constraints on dark energy
    Wang, Yun
    PHYSICAL REVIEW D, 2008, 78 (12):
  • [48] Repository for extended dark matter object constraints
    Croon, Djuna
    Munoz, Sergio Sevillano
    EUROPEAN PHYSICAL JOURNAL C, 2025, 85 (01):
  • [49] Complex dark photon dark matter EFT
    Bertuzzo, Enrico
    Sassi, Tommaso
    Tesi, Andrea
    JOURNAL OF HIGH ENERGY PHYSICS, 2024, (10):
  • [50] Model-independent approach for dark matter phenomenology: Signatures in linear colliders and cosmic positron experiments
    Shigeki Matsumoto
    Nobuchika Okada
    Pramana, 2007, 69 : 835 - 838