Search results for "Bolometers"

showing 5 items of 5 documents

CESAR: Cryogenic Electronics for Space Applications

2013

Ultra-low temperature sensors provide unprecedented performances in X-ray and far infrared astronomy by taking advantage of physical properties of matter close to absolute zero. CESAR is an FP7 funded project started in December 2010, that gathers six European laboratories around the development of high performances cryogenic electronics. The goal of the project is to provide far-IR, X-ray and magnetic sensors with signal-processing capabilities at the heart of the detectors. We present the major steps that constitute the CESAR work, and the main results achieved so far.

Far-infrared bolometersHEMTSNanotechnologyFar-infrared astronomySpace (mathematics)01 natural sciences030218 nuclear medicine & medical imagingNOISE03 medical and health sciencesCryogenic electronics0302 clinical medicineDevelopment (topology)Settore FIS/05 - Astronomia E Astrofisica0103 physical sciencesHigh impedance detectorsGeneral Materials ScienceElectronics4.2 KVOLTAGEAerospace engineering010302 applied physicsPhysicsbusiness.industryDetectorX-ray microcalorimetersCondensed Matter PhysicsAtomic and Molecular Physics and OpticsCryogenic electronics · High impedance detectors · X-ray microcalorimeters · Far-infrared bolometers1 KHZ[PHYS.COND.CM-MS]Physics [physics]/Condensed Matter [cond-mat]/Materials Science [cond-mat.mtrl-sci]business
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Precise measurement of $2\nu\beta\beta$ decay of $^{100}$Mo with the CUPID-Mo detection technology

2020

We report the measurement of the two-neutrino double-beta ($2\nu\beta\beta$) decay of $^{100}$Mo to the ground state of $^{100}$Ru using lithium molybdate (\crystal) scintillating bolometers. The detectors were developed for the CUPID-Mo program and operated at the EDELWEISS-III low background facility in the Modane underground laboratory. From a total exposure of $42.235$ kg$\times$d, the half-life of $^{100}$Mo is determined to be $T_{1/2}^{2\nu}=[7.12^{+0.18}_{-0.14}\,\mathrm{(stat.)}\pm0.10\,\mathrm{(syst.)}]\times10^{18}$ years. This is the most accurate determination of the $2\nu\beta\beta$ half-life of $^{100}$Mo to date. We also confirm, with the statistical significance of $>3\sigm…

Lithium molybdatePhysics - Instrumentation and DetectorsPhysics and Astronomy (miscellaneous)Analytical chemistry[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]nucl-ex01 natural sciencesAtomicchemistry.chemical_compoundParticle and Plasma Physicstwo-neutrino double-beta decay scintillating bolometers0103 physical sciencesddc:530Beta (velocity)Nuclear[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010306 general physicsNuclear ExperimentEngineering (miscellaneous)physics.ins-detS076H2NPhysicsQuantum Physics010308 nuclear & particles physicsPhysicsMolecularBeta decayNuclear & Particles Physics3. Good healthchemistrydouble beta decays bolometersUnderground laboratoryGround state
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Neutrinoless Double-Electron Capture

2020

Double-beta processes play a key role in the exploration of neutrino and weak interaction properties, and in the searches for effects beyond the Standard Model. During the last half century many attempts were undertaken to search for double-beta decay with emission of two electrons, especially for its neutrinoless mode ($0\nu2\beta^-$), the latter being still not observed. Double-electron capture (2EC) was not in focus so far because of its in general lower transition probability. However, the rate of neutrinoless double-electron capture ($0\nu2$EC) can experience a resonance enhancement by many orders of magnitude in case the initial and final states are energetically degenerate. In the re…

Particle physicsNuclear TheoryAtomic Physics (physics.atom-ph)Electron capturePhysics beyond the Standard ModelFOS: Physical sciencesdouble beta decayGeneral Physics and Astronomyhiukkasfysiikka7. Clean energy01 natural sciencesResonance (particle physics)neutrinoless double beta decayPhysics - Atomic PhysicsNuclear Theory (nucl-th)High Energy Physics - Phenomenology (hep-ph)0103 physical sciencesNuclear MatrixRoad mapNuclear Experiment (nucl-ex)010306 general physicsNuclear theoryNuclear Experimentnuclear tests of fundamental interactionsPhysics010308 nuclear & particles physicsBeta DecayBolometersHigh Energy Physics - PhenomenologyPräzisionsexperimente - Abteilung BlaumNeutrinoydinfysiikka
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Quantitative thermoelastic stress analysis by means of low-cost setups

2020

Abstract A low-cost Thermoelastic Stress Analysis (TSA) experimental setup is proposed which uses an ordinary micro-bolometer and in-house developed signal processing scripts. The setup is evaluated by analysing the thermoelastic signal from a tensile and a SENT specimen made of stainless steel AISI 304L, and the bolometer performances are compared with those of a state of the art photon detector. Signal processing is based on off-line cross-correlation, using a self-reference signal which is retrieved from the acquired thermal data. Procedures are in particular developed to recognise, quantify and correct errors due to spectral leakage and loss of streamed frames. The thermoelastic signal …

Signal processingMaterials scienceMicro-bolometersAcoustics/dk/atira/pure/subjectarea/asjc/2500/2504/dk/atira/pure/subjectarea/asjc/2200/2208Crack-growth monitoringThermoelastic stress analysis02 engineering and technologyFatigue testing01 natural sciencesSignallaw.invention010309 opticsSettore ING-IND/14 - Progettazione Meccanica E Costruzione Di MacchineThermoelastic dampingData acquisitionlaw0103 physical sciencesCalibrationElectrical and Electronic EngineeringSpectral leakageStress intensity factorSignal processing/dk/atira/pure/subjectarea/asjc/3100/3107Mechanical EngineeringBolometer021001 nanoscience & nanotechnologyAtomic and Molecular Physics and OpticsElectronic Optical and Magnetic MaterialsIR-thermography/dk/atira/pure/subjectarea/asjc/2200/22100210 nano-technology
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Probing the radio emission from air showers with polarization measurements

2014

The emission of radio waves from air showers has been attributed to the so-called geomagnetic emission process. At frequencies around 50 MHz this process leads to coherent radiation which can be observed with rather simple setups. The direction of the electric field induced by this emission process depends only on the local magnetic field vector and on the incoming direction of the air shower. We report on measurements of the electric field vector where, in addition to this geomagnetic component, another component has been observed which cannot be described by the geomagnetic emission process. The data provide strong evidence that the other electric field component is polarized radially wit…

SignalsAstronomy01 natural sciencesElectric fieldComputational physicsCosmic-raysComposition energy spectra and interactionscosmic rayRadio wavePhysicsEarth's magnetic fieldHigh Energy Astrophysical Phenomena (astro-ph.HE)Radiation[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph][SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PhysicsAstrophysics::Instrumentation and Methods for AstrophysicsPolarization (waves)Polarization (waves)BolometersThunderstormsMagnetic fieldComputingMethodologies_DOCUMENTANDTEXTPROCESSINGFísica nuclearAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaCAMPO MAGNÉTICOradio emissionRadio waveNuclear and High Energy Physics[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE][PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Air showerComposition energy spectra and interactions; Solar electromagnetic emission; BolometersAstrophysics::High Energy Astrophysical Phenomenainfrared submillimeter wave microwave and radiowave receivers and detectorsFieldFOS: Physical sciencesPierre Auger Observatory ; air shower ; radio emissionRadiationMonte-carlo SimulationsOpticsElectric field0103 physical sciencesddc:530Pierre auger observatory010306 general physicsPulsesInstrumentation and Methods for Astrophysics (astro-ph.IM)Pierre Auger Observatory010308 nuclear & particles physicsbusiness.industrySolar electromagnetic emissionFísicaOpticsDetectorComputational physics[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Air showerEarth's magnetic fieldMagnetic fieldExperimental High Energy PhysicsbusinessCodalema
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