The dark-PMT: A novel directional light dark matter detector based on vertically-aligned carbon nanotubes
The ANDROMeDa project, recently funded by the italian ministry of research with a 1M€grant, has the objective of developing, over the course of the next three years, a novel dark matter (DM) detector based on carbon nanotubes: the ‘dark-PMT’. Such a detector would be sensitive to DM-electron recoils...
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| Published in: | Nuclear instruments & methods in physics research. Section A, Accelerators, spectrometers, detectors and associated equipment Vol. 1050; p. 168116 |
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01-05-2023
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| Abstract | The ANDROMeDa project, recently funded by the italian ministry of research with a 1M€grant, has the objective of developing, over the course of the next three years, a novel dark matter (DM) detector based on carbon nanotubes: the ‘dark-PMT’. Such a detector would be sensitive to DM-electron recoils in the eV energy range, and could have world-leading sensitivity for DM masses below 30 MeV with an exposure of only 1g⋅year. Significant R&D is needed to produce carbon nanotubes with ideal properties for a DM target. In particular two by-products of synthesis (non-aligned crust layer and the sub-μm ‘waviness’) are expected to reduce electron transmission probability, and therefore need to be minimized. This will be done via a precise tuning of the evaporation and growth parameters, and of post-growth plasma etching. |
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| AbstractList | The ANDROMeDa project, recently funded by the italian ministry of research with a 1M€grant, has the objective of developing, over the course of the next three years, a novel dark matter (DM) detector based on carbon nanotubes: the ‘dark-PMT’. Such a detector would be sensitive to DM-electron recoils in the eV energy range, and could have world-leading sensitivity for DM masses below 30 MeV with an exposure of only 1g⋅year. Significant R&D is needed to produce carbon nanotubes with ideal properties for a DM target. In particular two by-products of synthesis (non-aligned crust layer and the sub-μm ‘waviness’) are expected to reduce electron transmission probability, and therefore need to be minimized. This will be done via a precise tuning of the evaporation and growth parameters, and of post-growth plasma etching. |
| ArticleNumber | 168116 |
| Author | Ruocco, Alessandro Pandolfi, Francesco Apponi, Alice Rago, Ilaria Mariani, Carlo Cavoto, Gianluca |
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| Cites_doi | 10.1016/j.ppnp.2019.02.004 10.1088/1475-7516/2019/07/047 10.1103/PhysRevLett.113.171301 10.1103/PhysRevLett.123.251801 10.1088/1361-6501/ac3d07 10.1088/1748-0221/17/05/P05021 10.1002/adbi.201800286 10.1109/TNS.2010.2047752 10.1016/j.apsusc.2012.12.129 10.1016/j.carbon.2018.07.032 10.1016/j.physletb.2017.11.064 10.1088/1748-0221/15/11/P11015 10.1021/jp073218h |
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| Title | The dark-PMT: A novel directional light dark matter detector based on vertically-aligned carbon nanotubes |
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