Search for Low-Mass Dark Matter with NEWS-G
University of Birmingham, Particle Physics Seminar, 6th November 2019
- P. Knights
University of Birmingham, UK and IRFU, CEA Saclay, France
06/11/2019 1 P Knights, UoB Particle Physics Seminar
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news-g.org Search for Low-Mass Dark Matter with NEWS-G University of Birmingham, Particle Physics Seminar, 6 th November 2019 P. Knights University of Birmingham, UK and IRFU, CEA Saclay, France P Knights, UoB Particle Physics Seminar
University of Birmingham, Particle Physics Seminar, 6th November 2019
University of Birmingham, UK and IRFU, CEA Saclay, France
06/11/2019 1 P Knights, UoB Particle Physics Seminar
news-g.org
P Knights, Particle Physics Seminar 06/11/2019
2 Astrophys.J. 648 (2006) L109-L113 Astrophys.J. 238 (1980) 471 Astrophys.J. 295 (1985) 305-313 Astron.Astrophys. 498 (2009) L33
Bullet Cluster Coma Cluster
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3 JCAP 1008 (2010) 004 J.Phys. G41 (2014) 063101
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4 J.Phys. G43 (2016) no.1, 013001
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I.Giomataris et al, JINST, 2008, P09007
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spherical proportional counter in CEA Saclay (sphere was previously a LEP RF cavity) Birmingham CEA Saclay SEDINE, LSM France
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⌀6.3 mm Anode SEDINE 8 cm Cu 15 cm Lead 30 cm Polyethelyne 5 μ/m2/day (Surface: ~14x106 μ/m2/day)
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10 Astropart.Phys. 97 (2018) 54-62
NEWS-G
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11 Astropart.Phys. 97 (2018) 54-62
NEWS-G
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J.Phys. G43 (2016) no.1, 013001
0.25 μ/m2/day 5 μ/m2/day
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Assumptions Flat background of 1.78 dru Exposure of 20 kg*days Energy window [14 eVee, 1 keVee] F=0.2, θ=0.12 SRIM quenching factor
Preliminary
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Assumptions Flat background of 1.78 dru Exposure of 20 kg*days Energy window [14 eVee, 1 keVee] F=0.2, θ=0.12 SRIM quenching factor
Preliminary
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(1) Cosmic Muons, (2) X-rays near shell, (3) X-rays in volume
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(1) Cosmic Muons, (2) X-rays near shell, (3) X-rays in volume
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I.Katsioulas et al, JINST, 13, 2018, no.11, P11006
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For rc =15 cm, ra = 1 mm, d = 3 mm, l = 20 mm, V1 = 2000 V
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55Fe source placed inside detector
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55Fe Source placed in two locations
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ACHINOS for SNOGLOBE
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Assumptions Flat background of 1.78 dru Exposure of 20 kg*days Energy window [14 eVee, 1 keVee] F=0.2, θ=0.12 SRIM quenching factor
Preliminary
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*Pacific Northwest National Laboratory, USA
63Cu(n,⍺)60Co by fast neutrons
238U and 232Th decay chain –
238U and 232Th measured directly
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*Pacific Northwest National Laboratory, USA
63Cu(n,⍺)60Co by fast neutrons
238U and 232Th decay chain –
238U and 232Th measured directly
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https://www.xia.com/ultralo-theory.html
222Rn during production 210Pb in our 4N copper: 28.5±8 mBq/kg
Nucl.Instrum.Meth. A884 (2018) 157-161
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Adv.High Energy Phys. 2014 (2014) 365432
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More on surface preparation: https://doi.org/10.1016/j.nima.2007.04.101
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Cu Movement in Electropolishing Cu Movement in Electroplating ~0.036 mm/day ~1.3 cm/year
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Assumptions Flat background of 1.78 dru Exposure of 20 kg*days Energy window [14 eVee, 1 keVee] F=0.2, θ=0.12 SRIM quenching factor
Preliminary
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Previous Limiting factors: ➔ Wall effect ➔ Sparking - Instability ➔ Low pressure ➔ Impurities ➔ Charge collection efficiency
14N + n → 14C + p + 625 keV, σth= 1.83 b 14N + n → 11B + α - 159 keV
239Pu
5.155 MeV
241Am
5.486 MeV
244Cm
5.805 MeV
Ar:CH4(98:2) 1000 mbar
239Pu
5.155 MeV
241Am
5.486 MeV
244Cm
5.805 MeV
N2 300 mbar
Neutron Beam 0.025 eV/ 4 MeV Proton Tracks Simulation Parameters: ∅ vessel 30 cm Nitrogen at 300 mbar Anode Ø 2 mm
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Aluminium S30
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+ MSci and Summer Students
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