\begin{document}$ 2\nu\beta\beta $\end{document}) and neutrinoless (\begin{document}$ 0\nu\beta\beta $\end{document}) decay modes, for five nuclei of the most experimental interest. Further, using the most recent experimental limits for \begin{document}$ 0\nu\beta\beta $\end{document} decay half-lives, we provide new constraints on the light mass neutrino parameter. Finally, by separating the factor representing the axial-vector constant to the forth power in the half-life formulas, we advance suggestions on how to reduce the errors introduced in the calculation by the uncertain value of this constant, exploiting the DBD data obtained from different isotopes and/or decay modes."> Computation of products of phase space factors and nuclear matrix elements for double beta decay -
  • [1]

    J. Vergados, H. Ejiri, and F. Simkovic, Rep. Prog. Phys.,75: 106301 (2012)

  • [2]

    F. T. Avignon, S.R. Elliott, and J. Engel, Rev. Mod. Phys.,80: 481 (2008)

  • [3]

    J. Suhonen and O. Civitarese, Phys. Rep.,300: 123 (1998)

  • [4]

    J. Kotila and F. Iachello, Phys. Rev. C,85: 034316 (2012)

  • [5]

    S. Stoica and M. Mirea, Phys. Rev. C,88: 037303 (2013)

  • [6]

    V. A. Rodin, A. Faessler, F. Simkovic et al, Phys. Rev. C,68: 044302 (2003); Nucl. Phys. A,793(2007)

  • [7]

    M. Kortelainen and J. Suhonen, Phys. Rev. C,75: 051303 (2007)

  • [8]

    F. Simkovic, A. Faessler, V. A. Rodin et al, Phys. Rev. C,77: 045503 (2008)

  • [9]

    F. Simkovic, A. Faessler, H. Muther et al, Phys. Rev. C,79: 055501 (2009)

  • [10]

    S. Stoica and H. V. Klapdor-Kleingrothaus, Nucl. Phys. A,694: 269 (2001)

  • [11]

    E. Caurier, J. Menendez, F. Nowacki et al, Phys. Rev.Lett.,100: 052503 (2008)

  • [12]

    J. Menendez, A. Poves, E. Caurier et al, Nuclear Physics A,818: 139 (2009)

  • [13]

    M. Horoi, S. Stoica and B.A. Brown, Phys. Rev. C, (2007)

  • [14]

    M. Horoi and S. Stoica, Phys. Rev.,81: 024321-024328 (2010)

  • [15]

    J. Barea and F. Iachello, Phys. Rev. C,79: 044301 (2009)

  • [16]

    J. Barea, J. Kotila, F. Iachello, Phys. Rev. C,87: 014315 (2013)

  • [17]

    J. Kotila and F. Iachello, Phys. Rev. C,87: 024313 (2013)

  • [18]

    P. K. Rath, R. Chandra, K. Chaturvedi et al, Phys. Rev. C,82: 064310 (2010)

  • [19]

    T. R. Rodriguez and G. Martinez-Pinedo, Phys. Rev. Lett,105: 252503 (2010)

  • [20]

    H. Primakov and S. P. Rosen, Rep. Prog. Phys.,22: 121 (1959)

  • [21]

    W. C. Haxton and G. J. Stephenson Jr., Prog. Theor. Part. Nucl. Phys.,12: 409 (1984)

  • [22]

    M. Doi, T. Kotani, H. Nishiura et al, Prog. Theor. Phys.,69: 602 (1983)

  • [23]

    M. Doi, T. Kotani, and E. Takasugi, Prog. Theor. Phys. Suppl.,83: 1 (1985)

  • [24]

    M. Doi and T. Kotani, Prog. Theor. Phys.,87: 1207 (1992)

  • [25]

    T. Tomoda, Rep. Prog. Phys.,54: 53 (1991)

  • [26]

    M. Mirea, T. E. Pahomi, and S. Stoica, Rom. Rep. Phys.,67: 872 (2015)

  • [27]

    M. Honma, T. Otsuka, B. A. Brown et al, Phys.Rev. C,69: 034335 (2004)

  • [28]

    M. Honma, T. Otsuka, T. Mizusaki et al, Phys. Rev. C,80: 064323 (2009)

  • [29]

    E. Caurier, F. Nowacki, and A. Poves, Phys. Rev. C,80: 048501 (2009)

  • [30]

    R. Arnold et al (NEMO3 Collaboration), Phys. Rev. D,93: 112008 (2016)

  • [31]

    C. Patrignani et al, Chin. Phys. C (PDG),40: 100001 (2016)

  • [32]

    CUORE, Eur. Phys. J. C,77: 857 (2017)

  • [33]

    Y. Iwata et al, Phys. Rev. Lett.,116: 112502 (2016)

  • [34]

    E. Caurier, F. Nowaki, and A. Poves, Phys. Lett. B,711: 62 (2012)

  • [35]

    S. F. King and C. Luhn, Rep. Prog. Phys.,76: 056201 (2013)

  • [36]

    A. Neacsu and S. Stoica, J. Phys. G,41: 015201 (2014)

  • [37]

    C. Giusti, H. Muther, F. D. Pacati et al, Phys. Rev. C,60: 054608 (1999)

  • [38]

    GERDA Collaboration, Phys. Rev. Lett.,120: 132503 (2018)

  • [39]

    V.I. Tretyak, NEMO3, AIP Conf. Proc.,1417: 125 (2011)

  • [40]

    CUORE Collaboration, Phys. Rev. Lett.,115: 102502 (2015)

  • [41]

    EXO Collaboration, Phys. Rev. Lett.,510: 229 (2018)

  • [42]

    F. Simkovic, R. Dvornicky, D. Stefanik et al, Phys. Rev. C,97: 034315 (2018)

  • [43]

    Y. Ren and Z. Ren, Phys. Rev. C,89: 064603 (2014)

Baidu
map