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000359718 0247_ $$2datacite_doi$$a10.15120/GSI-2025-00774
000359718 037__ $$aGSI-2025-00774
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000359718 088__ $$2Other$$a2022
000359718 1001_ $$0P:(DE-HGF)0$$aCBM Collaboration$$b0$$eCollaboration author
000359718 245__ $$amCBM@SIS18 2023/24
000359718 260__ $$aDarmstadt$$bGSI Helmholtzzentrum für Schwerionenforschung GmbH$$c2025
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000359718 4900_ $$aCBM Proposals
000359718 520__ $$aThis beam time application submitted in June 2022 is a continuation request by the CBM Collaboration to the General Program Advisory Committee (G-PAC) of GSI/FAIR, following the proposals which were granted in 2017 [4] and 2020 [5] within the FAIR phase-0 program of GSI / FAIR. The primary aim of mCBM@SIS18 (short “mCBM”) is to commission and optimize the complex interplay of the different detector systems with the triggerless-streaming data acquisition and the fast online event reconstruction and selection under realistic experiment conditions up to the top CBM interaction rate of 10 MHz. To validate the read-out and data processing concept of CBM the Λ production yield in Au + Au and Ni + Ni collisions at top SIS18 energies are measured with mCBM as a benchmark observable, which will allow comparison with published data by the FOPI and HADES experiment.
000359718 536__ $$0G:(DE-HGF)POF4-612$$a612 - Cosmic Matter in the Laboratory (POF4-612)$$cPOF4-612$$fPOF IV$$x0
000359718 693__ $$0EXP:(DE-Ds200)G-22-00110-20221208$$1EXP:(DE-Ds200)X0-20200803$$5EXP:(DE-Ds200)G-22-00110-20221208$$aX0$$eG-22-00110: mCBM@SIS18 2023/24 (Station: HTD,X0)$$x0
000359718 7001_ $$0P:(DE-Ds200)OR0467$$aHerrmann, Norbert$$b1$$eCorresponding author$$ugsi
000359718 7001_ $$0P:(DE-Ds200)OR1261$$aSturm, Christian$$b2$$eCorresponding author$$ugsi
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000359718 9131_ $$0G:(DE-HGF)POF4-612$$1G:(DE-HGF)POF4-610$$2G:(DE-HGF)POF4-600$$3G:(DE-HGF)POF4$$4G:(DE-HGF)POF$$aDE-HGF$$bForschungsbereich Materie$$lMatter and the Universe$$vCosmic Matter in the Laboratory$$x0
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