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Indium Solar Neutrino Experiments

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Physics and Astrophysics of Neutrinos
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Abstract

The possibility of detecting low-energy solar neutrinos through inverse β-decay in 115In was first discussed by R. S. Raghavan [1] in 1976. An indium experiment has unique features in that it is possible to measure the energy spectrum of solar neutrinos above 125 keV in real time. Although a variety of ideas concerning indium detectors have been discussed from time to time, and sophisticated ideas have been presented on various occasions, no practical designs for indium detectors have yet been demonstrated. We focus on discussions of problems that stand in the way of realizing a viable experiment in section 3. A survey of past and present development projects of the detector is given in section 4. A practical detector design and detailed background considerations for a dedicated detector for 7Be-pep neutrino detection are given in section 5.

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References

  1. R. Raghavan, Phys. Rev. Lett. 37, 259 (1976).

    Article  ADS  Google Scholar 

  2. J. N. Bahcall and R. K. Ulrich, Rev. Mod. Phys., 60, 297 (1988) and references therein.

    Article  ADS  Google Scholar 

  3. J. N. Bahcall, “Neutrino Astrophysics”, Cambridge University Press (1989).

    Google Scholar 

  4. S. P. Mikheyev and A. Yu. Smirnov, Sov. J. Nucl. Phys. 42, 913 (1985);

    Google Scholar 

  5. L. Wolfenstein, Phys. Rev. D17, 2369 (1978);

    ADS  Google Scholar 

  6. L. Wolfenstein, Phys. Rev. D20, 2634 (1979).

    ADS  Google Scholar 

  7. The tables of M. E. Rose, in Beta and Gamma Spectroscopy, edited by K. Siegbahn(North-Holland, Amsterdam, 1955), p875 was used in the calculation made by R. Raghavan’s 1976 paper [1].

    Google Scholar 

  8. R. Raghavan, Phys. Rev. Lett. 37, 259 (1976).

    Article  ADS  Google Scholar 

  9. J. Rapaport et al., Phys. Rev. Letts. 54, 2325 (1985).

    Article  ADS  Google Scholar 

  10. L. W. Alvares, Physics Notes, Memo No. 767, Lawrence Radiation Lab (1973).

    Google Scholar 

  11. R. S. Raghavan, in Proceedings of Informal Conference on Status and Future of Solar Neutrino Research, edited by G. Friedlander (Brookhaven National Laboratory) Report No. 50879, Vol 2, p1 (1978).

    Google Scholar 

  12. W. C. Haxton, Phys. Rev. C38, 2474 (1988).

    ADS  Google Scholar 

  13. M. Cribier et al., Nucl. Instr. and Methods, A265, 574 (1988).

    Article  ADS  Google Scholar 

  14. L. Pfeiffer et al., Phys. Rev. Lett. 41, 63 (1978).

    Article  ADS  Google Scholar 

  15. L. Pfeiffer et al. , Phys. Rev. C19, 1035 (1979).

    ADS  Google Scholar 

  16. A. G. D. Payne and N. E. Booth, Nucl. Instr. and Meth. A288, 632 (1990).

    Article  ADS  Google Scholar 

  17. A. K. Drukier and R. Nest, Nucl. Instr. and Methods, A239, 605(1985).

    Article  ADS  Google Scholar 

  18. Y. Suzuki et al., Nucl. Instr. and Methods, A293, 615 (1990).

    Article  ADS  Google Scholar 

  19. K. Inoue et al. ICRR-Report-252–91–21, ICRR Univ. of Tokyo, August, 1991.

    Google Scholar 

  20. Dojindo Laboratories.

    Google Scholar 

  21. InCl3–4H2O(Indium tri-chloride tetra hydrate) is also resolved in water [see [16]]. The maximum indium loading of 35% was actually obtained. This indium contained water is very transparent and the density is 1.85g/cm3. The index of reflection is about 1.7. By adding CeCl3 to the indium loaded water as a wavelength shifter, 360 nm light emission through an 260 nm excitation by a xenon lump was obtained. The indium loaded heavy water can be used as a Cherenkov detector with Ce activator. But this cannot be used as a scintillator since the liquid does not have an energy transfer property.

    Google Scholar 

  22. R. S. Raghavan, in Proc. Conf. on Status and Future of Solar Neutrinos, ed by G. Friedlander(Brookhaven National Laboratory Report BNL-50879, 1979) vol. II, p1.

    Google Scholar 

  23. M. Spiro, in Proc. 4th Moriond Workshop on Massive Neutrinos in Astrophysics and in Particle Physics, ed. by Tran Thanh Van (Editions Frontieres, 1984) p311.

    Google Scholar 

  24. R. S. Raghavan, in Proc. of Neutrino ’81, ed. by R. J. Cenece et al. (Univ. of Hawaii, 1981) Vol I, p27.

    Google Scholar 

  25. Y. Suzuki, Report of Grant-in-Aid for Scientific Research, 1988, The Ministry of education, Science and Culture.

    Google Scholar 

  26. L. Gonzalez-Mestres and D. Perret-Gallix, LAPP-EXP-87–03.

    Google Scholar 

  27. K. Oka and H. Unoki, J. of Crystal Growth 64, 385 (83).

    Google Scholar 

  28. F. J. Avella et al., Soc. Solid State Sci. 114, 613 (1968).

    Google Scholar 

  29. L. Gonzalez-Mestres, in Low Temperature detectors for Neutrinos and Dark Matter IV, ed. by N. E. Booth and G. L. Salmon, (Editions Frontieres, 1992), p471.

    Google Scholar 

  30. M. Avenier et al., Nucl. Phys. B (Proc. Suppl.) 28A, 496, (1992).

    Article  ADS  Google Scholar 

  31. T. Inagaki, Proc of the first workshop on solar neutrino detection, KEK Report 86–7, December 1986, ed. by M. Sakuda and Y. Suzuki.

    Google Scholar 

  32. D. R. Kania et al., Appl. Phys. Lett., 44 (1984)105, and references therein.

    Article  ADS  Google Scholar 

  33. Y. Suzuki, Proc. of the Vllth Moriond Workshop, Neutrinos and Exotic phenomena in Particle Physics and in Astrophysics, Les Arcs, Savoie, January 23–30, 1988.

    Google Scholar 

  34. Y. Suzuki et al., Nucl. and Instr. and Method, A275, 142 (1989).

    Article  ADS  Google Scholar 

  35. J. C. Lund et al., Nucl. Instr. and Meth. A272, 885 (1988).

    Article  ADS  Google Scholar 

  36. G. Waysand, Proc. of the Moriond workshop on Massive Neutrinos, January 1984, Ed. by J. Tran Thanh Van, p319.

    Google Scholar 

  37. A. de Bellefon and P. Espigat, LPC 86/22.

    Google Scholar 

  38. L. Gonzalez-Mestres and D. Perret-Gallix, LAPP-EXP-84–05-TH-112.

    Google Scholar 

  39. L. Gonzalez-Mestres and D. Perret-Gallix, LAPP-EXP-88–01.

    Google Scholar 

  40. Booth et al., in Solar Neutrinos and Neutrino Astronomy, ed by M. L. Cherry et al., AIP Conf. Proc. No.126, p216 (1985).

    Google Scholar 

  41. N. E. Booth, Sci. Prog. Oxf. 71, 563 (1987).

    Google Scholar 

  42. N. E. Booth, Appl. Phys. Lett. 50, 293 (1987).

    Article  ADS  Google Scholar 

  43. N. E. Booth, in Proc. Int. Symposium on Neutrino Astrophysics, ed by Y. Suzuki and K. Nakamura, Kamioka/Takayama, October (1992).

    Google Scholar 

  44. C. A. Klein, J. Appl. Phys. 39, 2029 (1968).

    Article  ADS  Google Scholar 

  45. D. J. Goldie, in X-ray Detection by Superconducting Tunnel Junctions, ed. by A. Barone et al., (World Scientific,1991), p.98.

    Google Scholar 

  46. D. J. Goldie et al., in Low Temperature Detectors for Neutrinos and Dark Matter IV, ed. by N.E. Booth and G. L. Salmon (Editions Frontieres, 1992), p.245.

    Google Scholar 

  47. A. de Bellefon et al., DPhPE 89–17.

    Google Scholar 

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© 1994 Springer Japan

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Suzuki, Y., Inoue, K. (1994). Indium Solar Neutrino Experiments. In: Fukugita, M., Suzuki, A. (eds) Physics and Astrophysics of Neutrinos. Springer, Tokyo. https://doi.org/10.1007/978-4-431-67029-2_10

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  • DOI: https://doi.org/10.1007/978-4-431-67029-2_10

  • Publisher Name: Springer, Tokyo

  • Print ISBN: 978-4-431-67031-5

  • Online ISBN: 978-4-431-67029-2

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