\begin{document}$ I(J^P)=1(1/2^+) $\end{document} and \begin{document}$ I(J^P)=1(3/2^+) $\end{document} using two bottom-up approaches: the deformed background and static dilaton models. In both models, we consider a non-linear Regge trajectory extension motivated by the strange nature of Σ baryons. We find that both models describe these systems with an RMS error smaller than 10%. We also perform a configurational entropy calculation in both models to discuss hadronic stability."> Holographic bottom-up approach to Σ baryons -
  • [1]

    H. Boschi-Filho and N. R. F. Braga, Eur. Phys. J. C32, 529 (2004), arXiv: hep-th/0209080

  • [2]

    J. Erlich, E. Katz, D. T. Sonet al., Phys. Rev. Lett.95, 261602 (2005), arXiv: hepph/0501128

  • [3]

    G. F. de Teramond and S. J. Brodsky, Phys. Rev. Lett.94, 201601 (2005), arXiv: hep-th/0501022

  • [4]

    A. Karch, E. Katz, D. T. Sonet al., Phys. Rev. D74, 015005 (2006), arXiv: hep-ph/0602229

  • [5]

    B. Batell and T. Gherghetta, Phys. Rev. D78, 026002 (2008), arXiv: 0801.4383[hep-ph]

  • [6]

    C. A. Ballon Bayona, H. Boschi-Filho, N. R. F. Bragaet al, Phys. Rev. D77, 046002 (2008), arXiv: 0705.1529[hep-th]

  • [7]

    A. Vega, I. Schmidt, T. Gutscheet al., Phys. Rev. D83, 036001 (2011), arXiv: 1010.2815[hepph]

  • [8]

    T. Branz, T. Gutsche, V. E. Lyubovitskijet al., Phys. Rev. D82, 074022 (2010), arXiv: 1008.0268[hep-ph]

  • [9]

    S. S. Afonin, Int. J. Mod. Phys. A25, 5683 (2010), arXiv: 1001.3105[hep-ph]

  • [10]

    P. Colangelo, F. De Fazio, F. Giannuzziet al., Phys. Rev. D78, 055009 (2008), arXiv: 0807.1054[hep-ph]

  • [11]

    P. Colangelo, F. Giannuzzi, and S. Nicotri, Phys. Rev. D83, 035015 (2011), arXiv: 1008.3116[hep-ph]

  • [12]

    C. A. Ballon Bayona, H. Boschi-Filho, and N. R. F. Braga, JHEP03, 064 (2008), arXiv: 0711.0221[hep-th]

  • [13]

    T. Gutsche, V. E. Lyubovitskij, I. Schmidtet al., Phys. Rev. D85, 076003 (2012), arXiv: 1108.0346[hepph]

  • [14]

    D. Li, M. Huang, and Q.-S. Yan, Eur. Phys. J. C73, 2615 (2013), arXiv: 1206.2824[hep-th]

  • [15]

    D. Li and M. Huang, JHEP11, 088 (2013), arXiv: 1303.6929[hep-ph]

  • [16]

    D. Li, M. Huang, Y. Yanget al., JHEP02, 030 (2017), arXiv: 1610.04618[hep-th]

  • [17]

    A. Vega and M. A. Martin Contreras, Phys. Rev. D102, 036017 (2020), arXiv: 2005.04501[hep-ph]

  • [18]

    Z. Abidin and C. E. Carlson, Phys. Rev. D77, 095007 (2008), arXiv: 0801.3839[hep-ph]

  • [19]

    Z. Abidin and C. E. Carlson, Phys. Rev. D77, 115021 (2008), arXiv: 0804.0214[hep-ph]

  • [20]

    Z. Abidin and C. E. Carlson, Phys. Rev. D79, 115003 (2009), arXiv: 0903.4818[hep-ph]

  • [21]

    A. Watanabe and K. Suzuki, Phys. Rev. D89, 115015 (2014), arXiv: 1312.7114[hep-ph]

  • [22]

    N. R. F. Braga and A. Vega, Eur. Phys. J. C72, 2236 (2012), arXiv: 1110.2548[hep-ph]

  • [23]

    S. J. Brodsky and G. F. de Teramond, Phys. Rev. D77, 056007 (2008), arXiv: 0707.3859[hep-ph]

  • [24]

    G. F. de Teramond and S. J. Brodsky, Phys. Rev. Lett.102, 081601 (2009), arXiv: 0809.4899[hep-ph]

  • [25]

    S. J. Brodsky and G. F. de Teramond, Phys. Rev. D78, 025032 (2008), arXiv: 0804.0452[hep-ph]

  • [26]

    S. J. Brodsky and G. F. de Teramond, Phys. Rev. Lett.96, 201601 (2006), arXiv: hep-ph/0602252

  • [27]

    A. Vega, I. Schmidt, T. Branzet al., Phys. Rev. D80, 055014 (2009), arXiv: 0906.1220[hep-ph]

  • [28]

    R. S. Sufian, Phys. Rev. D96, 093007 (2017), arXiv: 1611.07031[hep-ph]

  • [29]

    D. Chakrabarti, C. Mondal, A. Mukherjeeet al., Phys. Rev. D102, 113011 (2020), arXiv: 2010.04215[hep-ph]

  • [30]

    M. Ahmady, S. Kaur, S. L. MacKayet al., Phys. Rev. D104, 074013 (2021), arXiv: 2108.03482[hep-ph]

  • [31]

    J.-K. Chen, Phys. Lett. B786, 477 (2018), arXiv: 1807.11003[hep-ph]

  • [32]

    J.-K. Chen, Eur. Phys. J. C78, 235 (2018)

  • [33]

    J.-K. Chen, Eur. Phys. J. C78, 648 (2018)

  • [34]

    H. R. Grigoryan, P. M. Hohler, and M. A. Stephanov, Phys. Rev. D82, 026005 (2010), arXiv: 1003.1138[hepph]

  • [35]

    N. R. F. Braga, M. A. Martin Contreras, and S. Diles, Phys. Lett. B763, 203 (2016), arXiv: 1507.04708[hep-th]

  • [36]

    M. A. Martin Contreras and A. Vega, Phys. Rev. D101, 046009 (2020), arXiv: 1910.10922[hep-th]

  • [37]

    N. R. F. Braga, L. F. Ferreira, and A. Vega, Phys. Lett. B774, 476 (2017), arXiv: 1709.05326[hep-ph]

  • [38]

    M. A. Martin Contreras and A. Vega, Phys. Rev. D102, 046007 (2020), arXiv: 2004.10286[hep-ph]

  • [39]

    M. A. Martin Contreras and A. Vega, Phys. Rev. D108, 126024 (2023), arXiv: 2309.02905[hep-ph]

  • [40]

    O. Andreev, Phys. Rev. D73, 107901 (2006), arXiv: hepth/0603170

  • [41]

    H. Forkel, M. Beyer, and T. Frederico, JHEP07, 077 (2007), arXiv: 0705.1857[hep-ph]

  • [42]

    E. Folco Capossoli, M. A. Martın Contreras, D. Liet al., Chin. Phys. C44, 064104 (2020), arXiv: 1903.06269[hep-ph]

  • [43]

    E. Folco Capossoli, M. A. Martın Contreras, D. Liet al., Phys. Rev. D102, 086004 (2020), arXiv: 2007.09283[hep-ph]

  • [44]

    M. A. M. Contreras, E. F. Capossoli, D. Liet al., Phys. Lett. B822, 136638 (2021), arXiv: 2108.05427[hep-ph]

  • [45]

    M. A. Martin Contreras, E. Folco Capossoli, D. Liet al., Nucl. Phys. B977, 115726 (2022), arXiv: 2104.04640[hep-ph]

  • [46]

    M. Gleiser and N. Stamatopoulos, Phys. Lett. B713, 304 (2012), arXiv: 1111.5597[hep-th]

  • [47]

    M. Gleiser and N. Stamatopoulos, Phys. Rev. D86, 045004 (2012), arXiv: 1205.3061[hep-th]

  • [48]

    M. Gleiser and D. Sowinski, Phys. Lett. B727, 272 (2013), arXiv: 1307.0530[hep-th]

  • [49]

    N. R. F. Braga and R. da Rocha, Phys. Lett. B767, 386 (2017), arXiv: 1612.03289[hep-th]

  • [50]

    N. R. F. Braga and R. a. da Rocha, Phys. Lett. B776, 78 (2018), arXiv: 1710.07383[hep-th]

  • [51]

    R. da Rocha, Phys. Rev. D103, 106027 (2021), arXiv: 2103.03924[hep-ph]

  • [52]

    W. Barreto and R. da Rocha, Phys. Rev. D105, 064049 (2022), arXiv: 2201.08324[hep-th]

  • [53]

    M. A. Martin Contreras, A. Vega, and S. Diles, Phys. Lett. B835, 137551 (2022), arXiv: 2206.01834[hep-ph]

  • [54]

    Y.-Q. Zhao and D. Hou, Phys. Lett. B847, 138271 (2023), arXiv: 2305.07087[hep-ph]

  • [55]

    M. A. Martin Contreras, A. Vega, and S. Diles, Phys. Lett. B854, 138723 (2024), arXiv: 2308.16007[hep-ph]

  • [56]

    A. Vega and I. Schmidt, Phys. Rev. D79, 055003 (2009), arXiv: 0811.4638[hep-ph]

  • [57]

    M. Valenzuela and J. Zanelli, SciPost Phys.16, 065 (2024), arXiv: 2305.00106[hep-th]

  • [58]

    J.-K. Chen, Eur. Phys. J. C84, 356 (2024), arXiv: 2302.06794[hep-ph]

  • [59]

    . L. Workmanet al. (Particle Data Group), PTEP2022, 083C01 (2022)

  • [60]

    A. V. Sarantsev, M. Matveev, V. A. Nikonovet al., Eur. Phys. J. A55, 180 (2019), arXiv: 1907.13387[nucl-ex]

  • [61]

    C. E. Shannon, The Bell System Technical Journal27, 379 (1948)

  • [62]

    N. R. F. Braga and O. C. Junqueira, Phys. Lett. B814, 136082 (2021), arXiv: 2010.00714[hep-th]

  • [63]

    M. Gleiser and N. Jiang, Phys. Rev. D92, 044046 (2015), arXiv: 1506.05722[gr-qc]

  • [64]

    E. Crosato, M. Prokopenko, and R. E. Spinney, Physical Review E100, (2019)

  • [65]

    A. E. Bernardini and R. da Rocha, Phys. Lett. B762, 107 (2016), arXiv: 1605.00294[hep-th]

  • [66]

    A. E. Bernardini, N. R. F. Braga, and R. da Rocha, Phys. Lett. B765, 81 (2017), arXiv: 1609.01258[hep-th]

  • [67]

    N. R. F. Braga, L. F. Ferreira, and R. a. Da Rocha, Phys. Lett. B787, 16 (2018), arXiv: 1808.10499[hep-ph]

  • [68]

    A. E. Bernardini and R. Da Rocha, Phys. Rev. D98, 126011 (2018), arXiv: 1809.10055[hep-th]

  • [69]

    L. F. Ferreira and R. Da Rocha, Phys. Rev. D99, 086001 (2019), arXiv: 1902.04534[hep-th]

  • [70]

    I. L. Shapiro, Universe8, 586 (2022), arXiv: 1611.02263[gr-qc]

  • [71]

    S. S. Afonin and T. D. Solomko, Eur. Phys. J. C82, 195 (2022), arXiv: 2106.01846[hep-th]

Baidu
map