KATRIN and the Cosmic Neutrino Background Amand Faessler University of Tuebingen Germany Amand Faessler, Rastislav Hodak, Sergey Kovalenko, Fedor Simkovic: arXiv: 1304.5632 [nucl-th] 20. April 2013. Cosmic Microwave Background Radiation (Photons in the Maximum 2 mm) Decoupling of the photons from matter about 300 000 years after the Big Bang,when the electron are captured by the protons and He4 nuclei and the universe gets neutral. Photons move freely. Penzias and Wilson; Bell Telephon Nobel Price 1978 Planck Satellite Temperature Fluctuations Comic Microwave Background (March 21. 2013) We know the size of the hot spots. Curvature of the Univers flat x x 1 1 x WMAP 2002 : 1.00 0.02 1 6 The Universe is flat. The density has the critical value: = 1.00+-0.02 We can only see till the sphere of the the last photonelectron scattering: ~14 x1012 light years Microwave Background Radiation Experiment T = 2.7255(6) Kelvin Black body radiation. Temperature adjusted (pdg 2012): T=2.7255(6) K The relative number abundance of the light nuclei formed in the big bang allows to determine the absolute baryon density and relative to the critical density (flat universe). Baryon = rBaryon/rcritical = 0.02h-2 = 0.04 nB = 0.22 m-3 eB = 210 MeV/m-3 h = 0.71 h2 = 0.5 Hubble-Konstant= H = 100 h [km/(sec Mpc)] Bh2 = 0.02 Planck‘s Black Body Radiation Decoupling of Photons and Neutrinos from Matter „Re“-combination of Electrons with Protons and a-Particles (1g out of 1.7x109 from upper tail) 3000 Kelvin; 300 000 years after Big Bang; e- + p neutral Hydrogen-Atom 2e- + a neutral Helium-Atom Photons move freely since 14x1012 years. Last sphere of scattering: Radius = 14x1012 light years. Today Tg = 2.7255(6) Kelvin independent of the direction. Neutrino Decoupling and Cosmic Neutrino Background For massless-massive Neutrinos: Estimate of Neutrino Decoupling Universe Expansion rate: H=(da/dt)/a ~ n Interaction rate: G ne-e+<svrelative> H = \sqrt{8p G rtotal /3} = \sqrt{8 p r/(3 MPlanck2)} = = O(T2) [1/time] G ~ T3 <GF2 p2 c=1> = T3 GF2 T2 = GF2 T5 [Energy = 1/time] hbar = h/(2p) = c = 1 Neutrino Decoupling G/H = ( kB T/ 1MeV)3 ~ 1 T(Neutrinos)decoupl ~ 1MeV ~ 1010 Kelvin; Today: 1.95 K Time after Big Bang: 1 Second Below T = 1 MeV: T(Photons)decoupling = 3000 Kelvin; heute: 2.7255 K Time(Photons)decoupling = 300 000 years (Energy=Mass)-Density of the Universe log r Radiation dominated: r ~ 1/a4 ~ 𝑇4=Stefan-Boltzmann Matter dominated: r ~ 1/a3 ~ T3 Dark Energy a(t)~1/T 1 MeV 1 eV 3000 K 1sec 3x104y 300 000 y n dec. g dec. 8x109 y Tg = 2.7255 K Tn = 1.95 K 1/Temp heute Tranformation from Mass to Flavor Eigenstates Hamburg, March 3. 2008. Mass of the Electron Neutrino? Tritium decay (Mainz + Troisk) With: Hamburg, March 3. 2008. Measurement of the upper Limit of the Neutrino Mass in Mainz: mn < 2.2 eV 95% C.L. Kurie-Plot Eur. Phys. J. C40 (2005) 447 mn 2>0 mn2 <0 Q = 18.562 keV Electron Energy Negatives Squares of the Measured Neutrino Masses Ch. Kraus, B. Bornschein, L. Bornschein, J. Bonn, B. Flatt, A. Kovalik, B. Ostrick, E. W. Otten, J. P. Schall, Th. Thümmler, Ch Weinheimer: Eur. Phys. J. C40 (2005) 447-468. Anihilation of Relic Neutrinos with extreme High Energy Neutrinos > 1022 eV Energy Momentum conservation: n1(GZK,4x1022 eV) + n2(CB) Z0(4x1022eV)burst 10p0, 2 nucleons, 17 p+- Neutrino E = 4x1022 eV nrelic Z0 Above GZK DGZK=50Mpc Anihilation below Greisen-Zatsepin-Kuzmin Radius of 50 Mpc Cosmic Radiation from Z-Burst expected at 1021 -1022eV Free magnetic floating cylinder with half n absorbing material The system rotates 90 degrees. Permanent Magnet Superconducting Magnet Thomas Müller pointed this out to me. A. Ringwald: arXiv:hepph/031157v1; 2003. One half n absorbing, the other sterile. Balanced. Cylinder shaped Search for Cosmic Neutrino Background CnB by Beta decay (KATRIN): Tritium Kurie-Plot of Beta and induced Beta Decay: n(CB) + 3H(1/2+) 3He (1/2+) + e- Infinite good resolution Q = 18.562 keV Resolution Mainz: 4 eV mn < 2.3 eV Emitted electron Resolution KATRIN: 0.93 eV mn < 0.2 eV 90% C.L. Fit parameters: mn2 and Q value meV Electron Energy 2xNeutrino Masses Additional fit: only intensity of CnB Search for Cosmic Neutrino Background CnB by Beta decay: 187Re Kurie-Plot of beta and induced beta Decay: n(CB) + 18775Re112(5/2+) 18776Os111(1/2-) + e- Infinite good resolution Q = 2.460 keV MARE-Genova: DE ~ 11 eV mn ~ 2 eV 90% C.L. Milano-Bicocca: DE ~24 eV mn ~ 3-4 eV Fit parameters: mn2 and Q value meV Emitted electron Electron Energy 2xNeutrino Masses Additional fit: only intensity of CnB Tritium Beta Decay: 3H 3He+e-+nce Neutrino Capture: n(relic) + 3H 3He + e- 20 mg(eff) of Tritium 2x1018 T2-Molecules: Nncapture(KATRIN) = 1.7x10-6 nn/<nn> [year-1] Every 590 000 years a count!! for <nn> = 56 cm-3 Kaboth, Formaggio, Monreal: Phys. Rev. D82 (2010) 062001 66 mg(eff) of Tritium 6.6x1018 T2-Molecules: Nncapture(KATRIN) =5.5x10-6 nn/<nn> (year-1) Every 180 000 years a count. (For nn = <nn>) Faessler et al.: J. Phys. G38 (2011) 075202 50mg(eff) of Tritium 5x1018 T2-Molecules Nncapture(KATRIN) = 4.2x10-6 nn/<nn>(year-1) Every 240 000 years a counts.(For nn= <nn>) Drexlin April 2013: 20mg(eff) of Tritium 2x1018 T2-Molecules Nncapture(KATRIN) = 1.7x10-6 nn/<nn>(year-1) Every 590 000 years a counts.(For nn= <nn>) Two Problems 1. Number of Events with average Neutrino Density of nne = 56 [ Electron-Neutrinos/cm-3] Katrin: 1 Count in 590 000 Years Gravitational Clustering of Neutrinos!!!??? 2. Energy Resolution (KATRIN) DE ~ 0.93 eV Kurie-Plot Emitted electron Resolution KATRIN: 0.93 eV mn < 0.2 eV 90% C.L. Fit parameters: mn2 and Q value meV Electron Energy 2xNeutrino Masses Additional fit: only intensity of CnB Gravitational Clustering of Dark Matter and Neutrinos in Galaxies Dunkle Materie ? Faktum erwartet Was kompensiert die Zentrifugalkraft? Gravitational Clustering of Neutrinos A. Ringwald, Y. Wong: arXiv:hep-ph/0408241; solved Vlasov eq. for n; Dark Matter from Navarro et al. Ap J490 (1997) 493 Virial Mass: Mvir = 5v2R/G; v = velocity in sight Circles: 1h-1 kpc; Pentagons: 10h-1 kpc; Squares: 100h-1 kpc; Triangles 1000h-1 kpc. h-1 = 1.4 The solar system is 8 kpc = 24 000 ly from the galactic center. Gravitational Clustering of Neutrinos R.Lazauskas,P. Vogel and C.Volpe, J. Phys.g. 35 (2008) 025001; Light neutrinos: Gravitate only on Mpc (50 Mpc Galaxy Cluster) scale: nn/<nn> ~ nb/<nb> ~ 103 – 104; <nb>= 0.22 10-6 cm-3 A. Ringwald and Y. Wong: Vlasov trajectory simulations Clustering on Galactic Scale possible nn/<nn> = nb/<nb> ~ 106 ; (R = 30 kpc) Nncapture(KATRIN) = 1.7x10-6 nn/<nn> (year-1) = 1.7 (170 for 2 milligram) [counts per year] R. Wigmans, Astroparticle Physics 19 (2003) 379 discusses up to: nn/<nn> = 1013 but for us unrealistic. n Capture: ne(relic) + 18775Re(5/2)+18776Os(1/2)- + eMARE Genova and Milano Main Contribution: n s(1/2); e- p(3/2) 760 grams of AgReO4 Nncapture(MARE) = 6.7x10-8 nn/<nn> [year-1] For nn = <nn>: Every 15 Million years a count. For: nn/<nn> = 106: Every 15 years a count. (KATRIN: 1.7 per year) Summary 1 • The Cosmic Microwave Background allows to study the Universe 300 000 year after the BB. • The Cosmic Neutrino Background 1 sec after the Big Bang (BB): Tn(today) = 1.95 Kelvin. • Extremly difficult to detect: Small Cross Section and low Density 56 n‘s/cm3 and low Energies (1.95 Kelvin = 2x10-4 eV). Summary 2 1. Average Density: nne = 56 [ Electron-Neutrinos/cm-3] Katrin (20 mg eff. mass 3H): 1 Count in 590 000 Years Gravitational Clustering of Neutrinos nn/<nn> < 106 1.7 counts (2 milligram of 3H 170 counts) per year. 2. Measure only an upper limit of nn Kurie-Plot Emitted electron Resolution KATRIN: .93 eV mn < 0.2 eV 90% C.L. Fit parameters: mn2 and Q value meV ENDE Electron Energy 2xNeutrino Masses Additional fit: only intensity of CnB