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Time-Modulation of Two-Body Weak Decays with Massive Neutrinos
- P. Kienle
Excellence Cluster “Universe” Technische Universität München
“Sunshine by Cooling”
- P. Kienle, Naturwissenschaften 88 (2001) 313
- P. Kienle
Time-Modulation of Two-Body Weak Decays with Massive Neutrinos P. - - PowerPoint PPT Presentation
Time-Modulation of Two-Body Weak Decays with Massive Neutrinos P. Kienle P. Kienle Excellence Cluster Universe Technische Universit t M nchen Excellence Cluster Universe Technische Universit t M nchen Sunshine by
EURORIB 10, June 7, 2010 P. Kienle
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M.Jung et al. Phys. Rev. Lett. 69 (1992)2164 Yu.A.Litvinov et al. Phys.Rev. Lett. 99 (2007) 262501
EURORIB 10, June 7, 2010 P. Kienle
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142Pm60+ , 122I52+ H- like ions
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Combiner- Station
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PRL 77 (1996) 3803
J.P. Schiffer, P. Kienle Could there be an Ordered Condensed State in Beams of Fully Stripped Heavy Ions?
∆v/v → 0; signal/ noise high Γ= (Z²e²/d)/kT ∼ 1 Order parameter
EURORIB 10, June 7, 2010 P. Kienle
∆q= 0 for EC, ßb decay ∆f ∼ -∆m =Q
EURORIB 10, June 7, 2010 P. Kienle
t= 0 injection time
T=7.06(8)s a=0.18(3) ∆E∼10-15eV T=7.10(22)s a=0.22(3) T=6.13(3) s a=0.16(2)
Yu.A. Litvinov et al., Physics Letters B 664 (2008) 162
122I
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λEC(t) = ( 1+aECcos(ωECt+φ) ∆E∼10-15eV ∼ Mm
GSI Report 2009
a(ω=0.9 s-1) =0.03(3) The ß+ branch of 142Pm, three times stronger than the EC branch and simultaneously observed with a modulation frequency ω = 0.90 s-1 and an amplitude a = 0.18(5), shows a vanishing small modulation amplitude a = 0.03(3)
Time following the injection in the ESR t in s Modulation amplitude a(ω) with ω in s-1 a(ω)
EURORIB 10, June 7, 2010 P. Kienle
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From energy and momentum conservation in both decay channels |ν1>, |ν2>
EURORIB 10, June 7, 2010 P. Kienle
θ12= 45° ↔ decay width Γ
Asymptotic observation: 2 Lorentz lines
The transition amplitude of the EC decay m → d +νe is given by the sum of the amplitudes A (m → d + νj) (t), with the mixing coefficient Uej taking into account that only electron neutrinos νe contribute to the transition amplitude. Assuming θ13 ~ 0 with only two neutrino mass Eigen-states. Ue1 = cosθ12, and Ue2 = sinθ12 In time dependent perturbation theory the partial amplitude A (m → d + νj) (t), is defined in the rest frame of the mother ion m by
EURORIB 10, June 7, 2010 P. Kienle
EURORIB 10, June 7, 2010 P. Kienle
EURORIB 10, June 7, 2010 P. Kienle
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→ EC
Difference to EC neutrino ∆m²(KL)=0.759(21)x10-4 eV² ∆m²(EC)=2.9x∆m²(KamLAND) Small amplitude problem ?!?
EURORIB 10, June 7, 2010 P. Kienle
140Ce, Z=58
Similar mass corrections expected for antineutrinos from fission products but opposite sign (mass increase) arXiv: 0804 1311 (nucl-th)
In case that the neutrinos are not observed all flavours α= e, μ ,τ contribute to the decay amplitude
(A. Gal, arXiv:0809.1213v4 [nucl-th]
Interference terms cancel due to unitarity of mixing matrix:
EURORIB 10, June 7, 2010 P. Kienle
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EURORIB 10, June 7, 2010 P. Kienle
142 59+
142 59+
142 59+
142 59+
30th harmonic
124th harmonic
the same decay: improvement by a factor of about 100 and ∆t = 32ms
EURORIB 10, June 7, 2010 P. Kienle
EURORIB 10, June 7, 2010 P. Kienle
t↑ Frequency (31.25 Hz /channel)→ Time (32ms / channel) → mother daughter mother daughter 32 ms / channel decay
EURORIB 10, June 7, 2010 P. Kienle
t↑ Frequency → mother daughter Time → daughter mother
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EURORIB 10, June 7, 2010 P. Kienle
142Pm and 122I (preliminary) were observed as neutrino
EURORIB 10, June 7, 2010 P. Kienle
Fabian, Th. Faestermann, H. Geissel, V. Ivanova, P. Kienle, Ch.Kozhuharov,
Yamaguchi, J Zmeskal