Presentation is loading. Please wait.

Presentation is loading. Please wait.

O Reactor antineutrinos in the world V. Chubakov 1, F. Mantovani 1, B. Ricci 1, J. Esposito 2, L. Ludhova 3 and S. Zavatarelli 4 1 Dip. di Fisica, Università.

Similar presentations


Presentation on theme: "O Reactor antineutrinos in the world V. Chubakov 1, F. Mantovani 1, B. Ricci 1, J. Esposito 2, L. Ludhova 3 and S. Zavatarelli 4 1 Dip. di Fisica, Università."— Presentation transcript:

1 o Reactor antineutrinos in the world V. Chubakov 1, F. Mantovani 1, B. Ricci 1, J. Esposito 2, L. Ludhova 3 and S. Zavatarelli 4 1 Dip. di Fisica, Università degli Studi di Ferrara and INFN-Ferrara, Italy 2 INFN, Laboratori Nazionali di Legnaro, Padova, Italy 3 INFN- Milano, Italy 4 INFN- Genova, Italy The High Energy Region (HER) has to be controlled by studying the different contributions from the nuclear reactors, if one wants to disentangle N geo- and N react in the Low Energy Region (LER) Signal Calculations Result: a world wide map Total uncertainties on predicted signal is about 5%, coming from mixing, anti -spectrum, fuel composition and thermal power Reactor signal in Low Energy Region, for different sites. React. signal and geo neutrino detection Conclusions and perspectives We calculated reactor anti- e signal all over the world, by taking into account updated data on nuclear plants, anti- e spectrum and e oscillation parameters. We compare reactor signal with geo-neutrino signal for different places in the world. Study of time variation of reactor signal is also possible (± 10% variation in summer/winter). Detailed study on the effect of exhausted fuel must be completed (we estimate a 2% increase in the signal). We calculated reactor anti- e signal all over the world, by taking into account updated data on nuclear plants, anti- e spectrum and e oscillation parameters. We compare reactor signal with geo-neutrino signal for different places in the world. Study of time variation of reactor signal is also possible (± 10% variation in summer/winter). Detailed study on the effect of exhausted fuel must be completed (we estimate a 2% increase in the signal). 1 3 5 6 Reactor antineutrinos are the main source of background in the detection of geo-neutrinos (i.e. anti- e from 238 U and 232 Th decay chains, present in the Earth interior) 3.31.8 [MeV] E 8 Why reactor antineutrinos ? d i =reactor distance d i =reactor distance P i =thermal power P i =thermal power LF= Load Factor [1] LF= Load Factor [1] p k = power fraction p k = power fraction Q k =energy released for fission [4] Q k =energy released for fission [4] k =reactor anti- neutrino spectrum [5] k =reactor anti- neutrino spectrum [5] P ee =  oscillation survival probability [2] P ee =  oscillation survival probability [2]  (E  )= cross section  (E  )= cross section anti- e +p -> e + +n E th =1.806 MeV [3] PHYSICS DETECTO REACTOR Many ingredients: neutrino physics, nuclear physics, reactor properties… Sites React. LER [TNU] Geo  (G) [6] [TNU] R LER /G FREJUS 138 (1±5%) 43±133.2 SUDBURY 47 “ 47 “51±100.92 GRAN SASSO 23 “ 23 “41±80.56 PYHASALMI 19 “ 19 “51±80.37 BAKSAN 9.8 “ 9.8 “51±80.19 DUSEL 8.0 “ 8.0 “53±80.15 KAMIOKA 6.7 “ 6.7 “34±60.20 CURACAO 2.5 “ 2.5 “32±60.078 HAWAII 0.90 “ 0.90 “12±40.073 Bibliography: [1] courtesy by J. Mandula,IAEA, International Atomic Energy Agency 2012. [4] M. Apollonio et al., Eur. Phys. J. C27, 331 (2003) [2]G.L. Fogli et al., Phys. Rev. D 84, 053007 (2011)[5]Th. A Mueller et al., Phys.Rev.C83:054615 (2011) [3]F.Vissani and A. Strumia, Phys.Lett.B564:42-54 (2003)[6]G. Fiorentini et al., Phys.Rept.453:117-172 (2007) NUCLEAR k = 235 U, 238 U, 239 Pu, 241 Pu (nuclear fuel) 4 Frejus requires a detailed knowledge of closeby reactors. Kamioka is at the moment a very good site. Hawaii and Curacao are ‘wonderful’ places also for geo- study. Frejus requires a detailed knowledge of closeby reactors. Kamioka is at the moment a very good site. Hawaii and Curacao are ‘wonderful’ places also for geo- study. Neutrino 2012 June 3-9, 2012 Kyoto, Japan R.B.  =100% efficiency  =100% efficiency  = 1 year  = 1 year N p =10 32 target protons kton liquid scintillator) N p =10 32 target protons (  1kton liquid scintillator) DETECTOR Reactor antineutrino events all over the world 32 [1 TNU=1 event/ 10 32 target protons /year] Current status http://pris.iaea.org/public/ Japan cores switched off 394 333 215 Nuclear power plants in the world 2 Total Thermal Power =1023 GW PWR BWRPHWR GCR LWGRFBR % Total Thermal Power 63; 17% 249; 69% 47; 7.7% 18; 2.6% 15; 3.5% 2;  1 % PWRPressurized (light) Water Reactor BWRBoiling Water Reactor PHWRPressurized Heavy Water Reactor GCR Gas Cooled Reactor LWGR Light Water Graphite mod. FBR Fast Breeder Reactor


Download ppt "O Reactor antineutrinos in the world V. Chubakov 1, F. Mantovani 1, B. Ricci 1, J. Esposito 2, L. Ludhova 3 and S. Zavatarelli 4 1 Dip. di Fisica, Università."

Similar presentations


Ads by Google