1. KamLAND Experiment Kamioka Liquid scintillator Anti-Neutrino Detector - Largest low-energy anti-neutrino detector built so far - Located at the site of former Kamiokande experiment - High concentration of nuclear reactors at the right distance

2. 1000 ton Liquid Scintillator Balloon made of transparent nylon/EVOH composite film, supported by cargo net structure. Stainless steel tank filled with paraffin oil (0.04% lighter than LS). 1325 17-inch + 554 20-inch PMT’s Photosensitive coverage ~ 34% 3mm thick acrylic wall: Rn barrier Water Cherenkov outer detector 225 – 20inch PMT’s

3. KamLAND Experiment Designed to detect: - anti-neutrino interactions via inverse beta decay of electron scattering - neutrinos from the Sun - terrestrial anti-neutrinos - anti-neutrinos from the past Supernova - exotic nucleon decay modes

4. Detecting anti-neutrinos at KamLAND d p e+e+ 0.5 MeV  2.2 MeV  n p 0.5 MeV  e e-e- Inverse beta decay The positron loses its energy, then annihilates with an electron. (it’s a very fast event ~ns, seen as a unique flash by detector, brightness proportional to the kinetic energy of the positron plus 2 annihilation gammas) The neutron first thermalizes then is captured by a proton with a mean capture time of ~200ms. Prompt Delayed

5. Event Reconstruction -- Sort out waveforms coming from various ATWD’s at various times and bundle them into events – performed by “event builder”( putting together waveforms that come from the same detector trigger ) ATWD – Analog Transient Waveform Digitizer -- Convert the waveforms into pulses and extract arrival times and collected charge (number of photoelectrons collected by PMT) -- Area under each pulse is integrated, which corresponds to collected charge of the pulse. The pulse with the largest friction of the total charge (at least 15%) is chosen as the true PMT pulse within the waveform. Time is determined from the pulse shape. -- Raw waveforms collected from ATWD’s present a list of voltages

6. Determining event vertices Assumed that interactions are point like events and that light is emitted isotropically from the interaction point Vertex determined using the pulse arrival times. Calibrated using sources deployed down the center of the detector.

7. Determining event energies Estimation of particle’s energy is based on the hit pattern and the amount of light collected in the event and depends both on the particle position and particle type. The “visible” energy is calculated from the number of photo-electrons correcting for position. The “real” energy is calculated from the visible energy correcting for Cherenkov photons and scintillation light quenching. Quenching is defined as saturation of the scintillation emission for highly ionizing particles. Described by Birks’s law. Cherenkov light is emitted whenever particle moves through the Medium with speed grater than speed of light in that medium. Estimation of the fraction of energy lost is based on Monte Carlo calculations.

8. Selecting electron anti-neutrinos Veto after muons R p, R d < 5.5m Δr < 1.6m 0.5μs < ΔT < 500μs 1.8MeV < E d < 2.6MeV 2.6MeV < E p < 8.5MeV e+e+ 0.5 MeV  2.2 MeV  0.5 MeV  Prompt Delayed

9. Modes of s 1/2 neutron disappearance from 12 C : Search of the neutron decay into invisible channels, e.g. neutrinos. ( branches predicted by nuclear model )

10. 3 -hit event in the KamLAND detector: 1. The first hit produced by monoenergetic  s with an energy of 3.35 MeV corresponding to the de-excitation of a 2 + level of 10 C and by slow down interactions of neutrons in the scintillator 2. Second hit is due to the neutron capture by hydrogen in the scintillator ( lifetime ~ 200  s ) 3. The third hit will be due to delayed  + decay of 10 C gs with lifetime of 27.8 s and detectable energy in the range 1.74 – 3.65 MeV