Abstract
In this work we have evaluated the neutrino (NS) and antineutrino (AS) scattering cross sections on \(^{18}\)O and the inclusive muon capture rates at low energies within the Quasiparticle Random Phase Approximation (QRPA) and Projected QRPA (PQRPA) models. We present the first study of \(^{18}\)O\((\nu _e,e^-)^{18}\)F and \(^{18}\)O\((\bar{\nu }_e,e^+)^{18}\)N cross sections. These reactions are an important nuclear input for astrophysical calculations such as the CNO cycle. We have employed the weak formalism developed in Krmpotić et al. (Phys Rev C 71:044319, 2005) to analyze neutrino/antineutrino-nucleus scattering. Within this formalism, the nuclear residual interaction is described by \(\delta \)-force previously employed to evaluate single and double beta decays in QRPA models. The adopted parametrization leads to good results for the inclusive muon capture: we reproduce the available experimental data for the rate and the Gamow–Teller strength in \(^{18}\)F. We compared our results for the NS and AS cross sections on \(^{18}\)O with other theoretical evaluations on \(^{16}\)O, since there are no experimental data available for the processes on \(^{18}\)O. We noticed that the cross sections present a similar behavior as a function of the neutrino/antineutrino energy. For NS and AS we observed that the PQRPA procedure yields cross sections smaller than QRPA. We show that the Pauli blocking has an important role in the distribution of the partial contributions and the presence of two neutrons over the closed shell yields to higher NS cross sections than the AS cross sections. For NS and AS, the largest contribution comes from allowed and first-forbidden transitions, respectively.
Similar content being viewed by others
Data Availability
This manuscript has no associated data or the data will not be deposited. [Authors’ comment: Our paper has no associated data or the data will not be deposited.]
Notes
On the other hand, Sagawa et al. [44] discuss that no convincing evidence has been found about the spin-triplet pairing correlations in nuclei, such as the Wigner energy term in the mass formula, the enhancement of neutron–proton pair transfer cross sections, the inversion of \(J = 0^+\) and \(J = 1^+\) states, and the large enhancement of GT strength in the low-energy region of \(N = Z\) and \(N = Z + 2\) nuclei.
We use here the angular momentum coupling scheme \(\vert (\frac{1}{2},l)j \rangle \) [3].
Private communication.
References
Y. Fukuda et al., Phys. Rev. Lett. 81, 1562 (1998)
J. Suhonen, From Nucleons to Nucleus: Concepts of Microscopic Nuclear Theory (Springer, Berlin, 2007)
V.S. dos Ferreira, F. Krmpotić, C.A. Barbero, A.R. Samana, Phys. Rev. C 96, 044322 (2017)
V.S. dos Ferreira, A.R. Samana, F. Krmpotić, M. Chiapparini, Phys. Rev. C 101, 044314 (2020)
K.K. Gaikwad, S. Singh, Y.S. Lee, Environ. Chem. Lett. 16, 523 (2018)
B.A. Brown, B.H. Wildenthal, Ann. Rev. Nucl. Part. Soc. 38, 29 (1988)
H. Miyake, A. Mizukami, Phys. Rev. C 41, 329 (1990)
H.G. Benson, J.M. Irvine, Proc. Phys. Soc. 89, 249 (1966)
W.H. Chung, Singapore J. Phys. 4, 15 (1987); Phys. Abs. 67730 (1987)
J.C. Wheeler, C. Sneden, J.W. Truran Jr., Ann. Rev. Astron. Astrophys. 27, 279 (1989)
M. Hino, K. Muto, T. Oda, Phys. Rev. C 37, 1328 (1988)
J.P.F. Sellschop, Nucl. Instrum. Meth. Phys. Res. B 29, 439 (1987)
H.J. Fischbeck, Bull. Am. Phys. Soc. 33, 1691 (1988)
G.M. Fuller, B.S. Meyer, Astrop. J. 453, 792 (1995)
A.M. Serenelli, M. Fukugita, APJ 632, L33–L36 (2005)
T. Suzuki, S. Chiba, T. Yoshida, T. Kajino, T. Otsuka, Phys. Rev. C 74, 034307 (2006)
W. Hauser, H. Feshbach, Phys. Rev. 87, 366 (1952)
E. Kolbe, K. Langanke, G. Martínez-Pinedo, P. Vogel, J. Phys. G Nucl. Part. Phys. 29, 2569 (2003)
F. Cappuzzello, M. Cavallaro, C. Agodi et al., Eur. Phys. J. A 51, 145 (2015)
G. McLaughlin, G.M. Fuller, Astrop. J. 455, 202 (1995)
Y.-Z. Qian, J. Wassweburg, Phys. Rep. 442, 237 (2007)
P. Vogel, M.R. Zirnbauer, Phys. Rev. Lett. 57, 3148 (1986)
N. Paar, D. Vretenar, T. Marketin, P. Ring, Phys. Rev. C 77, 024608 (2008)
F. Krmpotić, A. Samana, A. Mariano, Phys. Rev. C 71, 044319 (2005)
F. Krmpotić, A. Mariano, A. Samana, Phys. Lett. B 541, 298 (2002)
A.R. Samana, F. Krmpotić, C.A. Bertulani, Comp. Phys. Commun. 181, 1123 (2010)
E.V. Bugaev et al., Nucl. Phys. A 324, 350 (1979)
A. Aguilar, L.B. Auerbach, R.L. Burman, D.O. Caldwell, E.D. Church, A.K. Cochran et al., Phys. Rev. D 64, 112007 (2001)
A.R. Samana et al., New J. Phys. 10, 033007 (2008)
O. Civitarese, P.O. Hess, J.G. Hirsch, Phys. Lett. B 412, 1 (1997)
F. Krmpotić, A. Mariano, T.T.S. Kuo, K. Nakayama, Phys. Lett. B 319, 393 (1993)
D. Sande Santos et al., Proceedings of Science, Volume 142—XXXIV Edition of the Brazilian Workshop on Nuclear Physics (XXXIV BWNP), March 20, 2012. https://doi.org/10.22323/1.142.0120
A. Samana, F. Krmpotić, A. Mariano, R.Z. Funchal, Phys. Lett. B 642, 100 (2006)
T.W. Donnelly, W.C. Haxton, Atom. Data Nucl. Data Tables 23, 103 (1979)
T.W. Donnelly, R.D. Peccei, Phys. Rep. 50, 1 (1979)
T. Kuramoto, M. Fukugita, Y. Kohyama, K. Kubodera, Nucl. Phys. A 512, 711 (1990)
R.J. Blin-Stoyle, S.C.K. Nair, Adv. Phys. 15, 493 (1966)
H. Castillo, F. Krmpotić, Nucl. Phys. A 469, 637 (1987). (and references therein)
M.R. Azevedo, R.C. Ferreira, A.J. Dimarco et al., Braz. J. Phys 50, 57 (2020)
J.S. O’Connell, T.W. Donnelly, J.D. Walecka, Phys. Rev. C 6, 719 (1972)
A.R. Samana, F. Krmpotic, N. Paar, C.A. Bertulani, Phys. Rev. C 83, 024303 (2011)
M.-K. Cheoun, E. Ha, K.S. Kim, T. Kajino, J. Phys. G 37, 055101 (2010)
M.-K. Cheoun, E. Ha, T. Kajino, Phys. Rev. C 83, 028801 (2011)
H. Sagawa, C.L. Bai, G. Colò, Phys. Scr. 91, 083011 (2016)
J. Hirsch, F. Krmpotić, Phys. Rev. C 41, 792 (1990)
J. Hirsch, F. Krmpotić, Phys. Lett. B 246, 5 (1990)
F. Krmpotić, J. Hirsch, H. Dias, Nucl. Phys. A 542, 85 (1992)
A. Bohr, B.R. Mottelson, Nuclear Structure, vol. I (Benjamin, New York, 1969)
M. Wang et al., Chin. Phys. C 36, 1603 (2012)
K. Nakayama, A.P. Galeão, F. Krmpotić, Phys. Lett. B 114, 217 (1982)
W. Unkelbach, PhD Thesis, Jül-Spez-472 (1988)
I. Supek, Teorijska Fizika-Zagreb (1964)
K. Ikeda, Prog. Theor. Phys. 31, 434 (1964)
D.R. Tilley, H.R. Weller, C.M. Cheves, R.M. Chasteler, Nucl. Phys. A 595, 170 (1995)
S. Yoshida, Y. Utsuno, N. Shimizu, T. Otsuka, Phys. Rev. C 97, 054321 (2018)
V. Gillet, N.V. Mau, Nuc. Phys. 54, 321 (1964)
F. Krmpotić, S.S. Sharma, Nucl. Phys. A 572, 329 (1994)
H. Fujita, Y. Fujita, Y. Utsuno, K. Yoshida, T. Adachi, A. Algora et al., Phys. Rev. C 100, 034618 (2019)
E. Ha, M.-K. Cheoun, H. Sagawa, Prog. Theor. Exp. Phys. 2022, 043D01 (2022)
T. Suzuki, D.F. Measday, J.P. Roalsvig, Phys. Rev. C 35, 2212 (1987). (and references therein)
J.N. Bahcall, Neutrino Astrophysics (Cambridge University Press, Cambridge, 1989)
R. Lazauskas, C. Volpe, Nucl. Phys. A 792, 219 (2007)
T.T.S. Kuo, F. Krmpotić, Y. Tzeng, Phys. Rev. Lett. 78, 2708 (1997)
C. Volpe, Particle Physics on the Eve of LHC, pp. 146-153 (2009). https://doi.org/10.1142/9789812837592_0020
J.A. Halbelib, R.A. Sorensen, Nucl. Phys. A 98, 542 (1967)
Acknowledgements
A.R.S and M.S acknowledge the financial support of FAPESB (Fundação de Amparo à Pesquisa do Estado da Bahia), T.O. PIE0013/2016 and to UESC/PROPP 0010299-61. C.A.B. is fellow of the CONICET, CCT La Plata (Argentina) and thanks for partial support. We also thank N. Paar for providing us with the spe for \(^{18}\)O, evaluated within the DD-ME2 model. This work has been done as a part of the Project INCT-Física Nuclear e Aplicações, Project number 464898/2014-5.
Author information
Authors and Affiliations
Corresponding author
Additional information
Communicated by Takashi Nakatsukasa.
Appendices
Appendix A: Relationship F and G NME
In this appendix, we give the relationship for G particle-particle (pp) and F particle-hole (ph) nuclear matrix elements with a general residual interaction V (following the conventions from the Unkelbach’s thesis [51]):
with the antisymmetrized matrix element:
and \( \vert cd \rangle _a = \frac{1}{\sqrt{2}}[\vert c \rangle \vert d \rangle -\vert d \rangle \vert c \rangle . \) Here, we use the coupling \(\vert a \rangle \equiv \vert (\frac{1}{2}\ell _a)j_a \rangle \).
The particle-particle (PP) coupling is:
and the particle-hole (ph) coupling is:
where \(\vert a^{-1} \rangle =\textbf{a}\vert 0 \rangle =\vert (j_am_a)^{-1} \rangle =(-1)^{j_a-m_a} \vert j_a-m_a \rangle \).
The antisymmetrized pp state is:
with the property: \(\vert ab,J \rangle _a =(-1)^{j_a+j_b-J+1} \vert ba,J \rangle _a\).
The pp matrix element is defined as:
and the ph matrix element as:
where
Thus
The pp and the ph matrix elements are related as:
Appendix B: NME for \(\delta \)-force
The nuclear matrix elements for the \(\delta \)-residual interaction are taken from Ref. [52, 53]. They were used in several works describing single and double beta decay as well semileptonic interactions as muon capture decay and neutrino capture [3, 4, 24, 45,46,47]. Here, we give a brief summary of main results. The residual interaction \(\delta -\)force (in units of MeV.fm\(^3\))reads
where \(v_t\) and \( v_s \) are the singlet and triplet couplings constants in the pp and ph channels, respectively. The argument \(r=\vert \textbf{r}_1 -\textbf{r}_2 \vert \), and \(P_t\) and \(P_t\) are the spin and isospin-projection operators
with
are the spin-projection \(\Pi _S\) and isospin-projection operators \(\Lambda _T\).
From pg. 642 of Ref. [52] the matrix element for the \(\delta \)-force between non-identical particles are
and
where
Introducing the shorthand notation:
Finally, the matrices F and G for \(\delta \)-force residual interaction read
According to the hypothesis of Halbleib and Sorensen on the particle-hole force [65], the parameters \(v_s\) and \(v_t\) of the previous equations are different. For pp we have the t and s parameters defined in Eq. (23) related with \(v_t\) and \(v_t\) of Eq. (B17). While for the ph channel, we have the ph-coupling constants, \(v_s^\textrm{ph}\) and \(v_t^\textrm{ph}\) for Eq. (B18).
Rights and permissions
Springer Nature or its licensor (e.g. a society or other partner) holds exclusive rights to this article under a publishing agreement with the author(s) or other rightsholder(s); author self-archiving of the accepted manuscript version of this article is solely governed by the terms of such publishing agreement and applicable law.
About this article
Cite this article
Mohammadzadeh, M., Khalili, H., Samana, A.R. et al. Neutrino and Antineutrino captures on \(^{18}\)O within QRPA models. Eur. Phys. J. A 59, 31 (2023). https://doi.org/10.1140/epja/s10050-023-00944-6
Received:
Accepted:
Published:
DOI: https://doi.org/10.1140/epja/s10050-023-00944-6