First results from ABRACADABRA-10 cm: a search for Sub-eV axion dark matter
<|begin_of_text|><|start_header_id|>system<|end_header_id|> You are a research archivist expert in dataset metadata. Answer the question truthfully.  <|eot_id|><|start_header_id|>user<|end_header_id|> Here is the Description of a dataset. Description:'The axion is a promising dark matter candidate, which was originally proposed to solve the strong-CP problem in particle physics. To date, the available parameter space for axion and axion like particle dark matter is relatively unexplored, particularly at massesma ≲ 1 μeV.ABRACADABRAis a new experimental program to search for axion dark matter over a broad range of masses, 10−12 ≲ ma ≲ 10−6 eV. ABRACADABRA-10 cm is a small-scale prototype for a future detector that could be sensitive to the QCD axion. In this Letter, we present the first results from a 1 month search for axions with ABRACADABRA-10 cm. We find no evidence for axionlike cosmic dark matter and set 95% C.L. upper limits on the axion-photon coupling between gaγγ < 1.4 × 10−10 and gaγγ < 3.3 × 10−9 GeV−1 over the mass range 3.1 × 10−10–8.3 × 10−9 eV. These results are compet' . Please return only a json list of at most 3 Keywords corresponding to the Description:.<|eot_id|><|start_header_id|>assistant<|end_header_id|> {"Answer" : ["ABRACADABRA","available parameter space","axionlike cosmic dark matter","axionlike particle dark matter","axion-photon coupling","dark matter candidate","electron volt energy 1.0 mueV","mass range","particle physics","QCD axion","size 10.0 cm","strong-CP problem","time 1.0 month"]} <|eot_id|>
 Here is the Description of a dataset. Description:'The axion is a promising dark matter candidate, which was originally proposed to solve the strong-CP problem in particle physics. To date, the available parameter space for axion and axion like particle dark matter is relatively unexplored, particularly at massesma ≲ 1 μeV.ABRACADABRAis a new experimental program to search for axion dark matter over a broad range of masses, 10−12 ≲ ma ≲ 10−6 eV. ABRACADABRA-10 cm is a small-scale prototype for a future detector that could be sensitive to the QCD axion. In this Letter, we present the first results from a 1 month search for axions with ABRACADABRA-10 cm. We find no evidence for axionlike cosmic dark matter and set 95% C.L. upper limits on the axion-photon coupling between gaγγ < 1.4 × 10−10 and gaγγ < 3.3 × 10−9 GeV−1 over the mass range 3.1 × 10−10–8.3 × 10−9 eV. These results are compet' . Please return only a json list of at most 3 Keywords corresponding to the Description:.
The axion is a promising dark matter candidate, which was originally proposed to solve the strong-CP problem in particle physics. To date, the available parameter space for axion and axion like particle dark matter is relatively unexplored, particularly at massesma ≲ 1 μeV.ABRACADABRAis a new experimental program to search for axion dark matter over a broad range of masses, 10−12 ≲ ma ≲ 10−6 eV. ABRACADABRA-10 cm is a small-scale prototype for a future detector that could be sensitive to the QCD axion. In this Letter, we present the first results from a 1 month search for axions with ABRACADABRA-10 cm. We find no evidence for axionlike cosmic dark matter and set 95% C.L. upper limits on the axion-photon coupling between gaγγ < 1.4 × 10−10 and gaγγ < 3.3 × 10−9 GeV−1 over the mass range 3.1 × 10−10–8.3 × 10−9 eV. These results are compet
ABRACADABRA; available parameter space; axionlike cosmic dark matter; axionlike particle dark matter; axion-photon coupling; dark matter candidate; electron volt energy 1.0 mueV; mass range; particle physics; QCD axion; size 10.0 cm; strong-CP problem; time 1.0 month