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Energy calibration of the 2.5 MV Pelletron at the Dalton Cumbrian Facility.

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Title: Energy calibration of the 2.5 MV Pelletron at the Dalton Cumbrian Facility.
Authors: Linkowski, K.1 (AUTHOR), Sidhu, R. S.1,2 (AUTHOR) ragan.sidhu@surrey.ac.uk, Skowronski, J.3,4 (AUTHOR), Aliotta, M.1 (AUTHOR) m.aliotta@ed.ac.uk, Black, P.1 (AUTHOR), Davinson, T.1 (AUTHOR), Wiescher, M.1,5 (AUTHOR), Caciolli, A.3 (AUTHOR), Jones, J.1 (AUTHOR), Manukyan, K.5 (AUTHOR), Robertson, D.5 (AUTHOR), Smith, A.6 (AUTHOR)
Source: European Physical Journal A -- Hadrons & Nuclei. Jul2025, Vol. 61 Issue 7, p1-8. 8p.
Subjects: Nuclear astrophysics, Stellar evolution, Calibration, Nucleosynthesis, Proton beams, Laboratories, Linear accelerators
Abstract: We report on the energy calibration of the 2.5 MV Pelletron accelerator at the Dalton Cumbrian Facility in England (UK) using five well-known resonances in the 27Al(p, γ) 28 Si reaction in the proton beam energy range of 632–1800 keV. The beam energy spread was also measured and found to be 191(38) eV. Additionally, we checked the stability and reproducibility of the accelerator's beam energy, confirming its suitability for nuclear astrophysics experiments, especially in the high-energy regime of stellar evolution and nucleosynthesis. [ABSTRACT FROM AUTHOR]
Copyright of European Physical Journal A -- Hadrons & Nuclei is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
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  Data: Energy calibration of the 2.5 MV Pelletron at the Dalton Cumbrian Facility.
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  Data: <searchLink fieldCode="AR" term="%22Linkowski%2C+K%2E%22">Linkowski, K.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Sidhu%2C+R%2E+S%2E%22">Sidhu, R. S.</searchLink><relatesTo>1,2</relatesTo> (AUTHOR)<i> ragan.sidhu@surrey.ac.uk</i><br /><searchLink fieldCode="AR" term="%22Skowronski%2C+J%2E%22">Skowronski, J.</searchLink><relatesTo>3,4</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Aliotta%2C+M%2E%22">Aliotta, M.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<i> m.aliotta@ed.ac.uk</i><br /><searchLink fieldCode="AR" term="%22Black%2C+P%2E%22">Black, P.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Davinson%2C+T%2E%22">Davinson, T.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Wiescher%2C+M%2E%22">Wiescher, M.</searchLink><relatesTo>1,5</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Caciolli%2C+A%2E%22">Caciolli, A.</searchLink><relatesTo>3</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Jones%2C+J%2E%22">Jones, J.</searchLink><relatesTo>1</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Manukyan%2C+K%2E%22">Manukyan, K.</searchLink><relatesTo>5</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Robertson%2C+D%2E%22">Robertson, D.</searchLink><relatesTo>5</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Smith%2C+A%2E%22">Smith, A.</searchLink><relatesTo>6</relatesTo> (AUTHOR)
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  Data: <searchLink fieldCode="JN" term="%22European+Physical+Journal+A+--+Hadrons+%26+Nuclei%22">European Physical Journal A -- Hadrons & Nuclei</searchLink>. Jul2025, Vol. 61 Issue 7, p1-8. 8p.
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  Data: <searchLink fieldCode="DE" term="%22Nuclear+astrophysics%22">Nuclear astrophysics</searchLink><br /><searchLink fieldCode="DE" term="%22Stellar+evolution%22">Stellar evolution</searchLink><br /><searchLink fieldCode="DE" term="%22Calibration%22">Calibration</searchLink><br /><searchLink fieldCode="DE" term="%22Nucleosynthesis%22">Nucleosynthesis</searchLink><br /><searchLink fieldCode="DE" term="%22Proton+beams%22">Proton beams</searchLink><br /><searchLink fieldCode="DE" term="%22Laboratories%22">Laboratories</searchLink><br /><searchLink fieldCode="DE" term="%22Linear+accelerators%22">Linear accelerators</searchLink>
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  Data: We report on the energy calibration of the 2.5 MV Pelletron accelerator at the Dalton Cumbrian Facility in England (UK) using five well-known resonances in the 27Al(p, γ) 28 Si reaction in the proton beam energy range of 632–1800 keV. The beam energy spread was also measured and found to be 191(38) eV. Additionally, we checked the stability and reproducibility of the accelerator's beam energy, confirming its suitability for nuclear astrophysics experiments, especially in the high-energy regime of stellar evolution and nucleosynthesis. [ABSTRACT FROM AUTHOR]
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  Data: <i>Copyright of European Physical Journal A -- Hadrons & Nuclei is the property of Springer Nature and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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        Value: 10.1140/epja/s10050-025-01622-5
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      – Code: eng
        Text: English
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    Subjects:
      – SubjectFull: Nuclear astrophysics
        Type: general
      – SubjectFull: Stellar evolution
        Type: general
      – SubjectFull: Calibration
        Type: general
      – SubjectFull: Nucleosynthesis
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      – SubjectFull: Proton beams
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      – SubjectFull: Laboratories
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      – SubjectFull: Linear accelerators
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              Text: Jul2025
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