Bjoern Lehnert

Dr. Bjoern Lehnert

Nuclear Science Division, Lawrence Berkeley National Laboratory, Berkeley, CA 94720, USA
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Research Focus & Metrics

Academic Career Length

16Years (2011-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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29 March 2018 in The European Physical Journal Plus
Verified
Journal Article
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CAC. E. Aalseth
C. E. Aalseth
FAF. Acerbi
F. Acerbi
PAP. Agnes
P. Agnes
IAI. F. M. Albuquerque
I. F. M. Albuquerque
TAT. Alexander
T. Alexander
GZG. Zuzel
G. Zuzel

19 September 2013 in Physical Review Letters
Verified
Journal Article
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MAM. Agostini
M. Agostini
MAM. Allardt
M. Allardt
EAE. Andreotti
E. Andreotti
ABA. M. Bakalyarov
A. M. Bakalyarov
MBM. Balata
M. Balata
GZG. Zuzel
G. Zuzel
Neutrinoless double beta decay is a process that violates lepton number conservation. It is predicted to occur in extensions of the standard model of particle physics. This Letter reports the results from phase I of the Germanium Detector Array (GERDA) experiment at the Gran Sasso Laboratory (Italy) searching for neutrinoless double beta decay of the isotope Ge76. Data considered in the present analysis have been collected between November 2011 and May 2013 with a total exposure of 21.6 kg yr. A blind analysis is performed. The background index is about 1×10−2  counts/(keV kg yr) after pulse shape discrimination. No signal is observed and a lower limit is derived for the half-life of neutrinoless double beta decay of Ge76, T1/20ν>2.1×1025  yr (90% C.L.). The combination with the results from the previous experiments with Ge76 yields T1/20ν>3.0×1025  yr (90% C.L.).

1 March 2013 in The European Physical Journal C
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Journal Article
Open access
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KAK.-H. Ackermann
K.-H. Ackermann
MAM. Agostini
M. Agostini
MAM. Allardt
M. Allardt
MAM. Altmann
M. Altmann
EAE. Andreotti
E. Andreotti
GZG. Zuzel
G. Zuzel
The Gerda collaboration is performing a search for neutrinoless double beta decay of 76Ge with the eponymous detector. The experiment has been installed and commissioned at the Laboratori Nazionali...

1 March 2019 in Astroparticle Physics
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Journal Article
Closed access
PAP.-A. Amaudruz
P.-A. Amaudruz
MBM. Baldwin
M. Baldwin
MBM. Batygov
M. Batygov
BBB. Beltran
B. Beltran
CBC.E. Bina
C.E. Bina
JZJ. Zielinski
J. Zielinski

17 August 2018 in Physical Review Letters
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Journal Article
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PAP.-A. Amaudruz
P.-A. Amaudruz
MBM. Baldwin
M. Baldwin
MBM. Batygov
M. Batygov
BBB. Beltran
B. Beltran
CBC. E. Bina
C. E. Bina
DCDEAP-3600 Collaboration
DEAP-3600 Collaboration
This Letter reports the first results of a direct dark matter search with the DEAP-3600 single-phase liquid argon (LAr) detector. The experiment was performed 2 km underground at SNOLAB (Sudbury, Canada) utilizing a large target mass, with the LAr target contained in a spherical acrylic vessel of 3600 kg capacity. The LAr is viewed by an array of PMTs, which would register scintillation light produced by rare nuclear recoil signals induced by dark matter particle scattering. An analysis of 4.44 live days (fiducial exposure of 9.87 ton day) of data taken during the initial filling phase demonstrates the best electronic recoil rejection using pulse-shape discrimination in argon, with leakage <1.2×10−7 (90% C.L.) between 15 and 31  keVee. No candidate signal events are observed, which results in the leading limit on weakly interacting massive particle (WIMP)-nucleon spin-independent cross section on argon, <1.2×10−44  cm2 for a 100  GeV/c2 WIMP mass (90% C.L.).

7 August 2015 in Physical Review D
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Journal Article
Open access
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MAM. Agostini
M. Agostini
SAS. Appel
S. Appel
GBG. Bellini
G. Bellini
JBJ. Benziger
J. Benziger
DBD. Bick
D. Bick
BCBorexino Collaboration
Borexino Collaboration
We report an improved geoneutrino measurement with Borexino from 2056 days of data taking. The present exposure is (5.5±0.3)×1031  proton×yr. Assuming a chondritic Th/U mass ratio of 3.9, we obtain 23.7−5.7+6.5(stat)−0.6+0.9(sys) geoneutrino events. The null observation of geoneutrinos with Borexino alone has a probability of 3.6×10−9 (5.9σ). A geoneutrino signal from the mantle is obtained at 98% C.L. The radiogenic heat production for U and Th from the present best-fit result is restricted to the range 23–36 TW, taking into account the uncertainty on the distribution of heat producing elements inside the Earth.