Novel approach to infer the 2H⁡(𝑝,𝛾)⁢3He angular distribution: Experimental results and comparison with theoretical calculations

K Stockel; N. Mozumdar; S Zavatarelli; F Ferraro; M. Aliotta; C. Ananna; L. Barbieri; F Barile; D Bemmerer; A Best; A Boeltzig; C Broggini; C. G. Bruno; A Caciolli; M. Campostrini; F Cavanna; F. Casaburo; G F  Ciani; P Colombetti; A. Compagnucci; P Corvisiero; L. Csedreki; T. Davinson; R Depalo; D. Dell'Aquila; A Di Leva; Z Elekes; A Formicola; Zs Fulop; G Gervino; R Gesue; A Guglielmetti; C Gustavino; Gy Gyurky; A. Kievsky; G Imbriani; M Junker; M Lugaro; L. E. Marcucci; P Marigo; J. Marsh; E Masha; R Menegazzo; D Mercogliano; V Mossa; V Paticchio; D Piatti; P Prati; D. Rapagnani; V. Rigato; D. Robb; L Schiavulli; R.S. Sidhu; J. Skowronski; O Straniero; T Szucs; M. Viviani

doi:10.1103/PhysRevC.110.L032801

Novel approach to infer the 2H⁡(𝑝,𝛾)⁢3He angular distribution: Experimental results and comparison with theoretical calculations

K Stockel, N. Mozumdar, S Zavatarelli, F Ferraro, M. Aliotta, C. Ananna, L. Barbieri, F Barile, D Bemmerer, A Best, A Boeltzig, C Broggini, C. G. Bruno, A Caciolli, M. Campostrini, F Cavanna^*, F. Casaburo, G F Ciani, P Colombetti, A. CompagnucciP Corvisiero, L. Csedreki, T. Davinson, R Depalo, D. Dell'Aquila, A Di Leva, Z Elekes, A Formicola, Zs Fulop, G Gervino, R Gesue, A Guglielmetti, C Gustavino^*, Gy Gyurky, A. Kievsky, G Imbriani, M Junker, M Lugaro, L. E. Marcucci, P Marigo, J. Marsh, E Masha, R Menegazzo, D Mercogliano, V Mossa, V Paticchio, D Piatti, P Prati, D. Rapagnani, V. Rigato, D. Robb, L Schiavulli, R.S. Sidhu, J. Skowronski, O Straniero, T Szucs, M. Viviani

^*Corresponding author for this work

School of Physics and Astronomy

Research output: Contribution to journal › Letter › peer-review

Abstract / Description of output

The D(p,γ)3He reaction is of primary importance in cosmology and nuclear physics since it offers a unique opportunity to test predictions based on the description of nuclear interactions. We present a novel approach to extract the angular distribution of the photons emitted by the D(p,γ)
3He reaction inferred from the shape of the experimental γ-spectra. The measurement was performed in the Gran Sasso Laboratories by the LUNA collaboration. By using a HPGe detector faced to an extended deuterium gas target, it was possible to derive the angular distribution in the 30-280 keV kinetic energy range and to compare the results with recent ab-initio predictions.

Original language	English
Article number	L032801
Pages (from-to)	1-7
Number of pages	7
Journal	Physical Review C
Volume	110
Issue number	3
DOIs	https://doi.org/10.1103/PhysRevC.110.L032801
Publication status	Published - 18 Sept 2024

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10.1103/PhysRevC.110.L032801

Stoeckel_LP1824126Accepted author manuscript, 588 KBLicence: Creative Commons: Attribution (CC-BY)

Edinburgh Nuclear Physics Group Consolidated Grant Proposal
Woods, P., Aliotta, M., Murphy, A. & Watts, D.
STFC
1/08/14 → 30/09/18
Project: Research

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Stockel, K., Mozumdar, N., Zavatarelli, S., Ferraro, F., Aliotta, M., Ananna, C., Barbieri, L., Barile, F., Bemmerer, D., Best, A., Boeltzig, A., Broggini, C., Bruno, C. G., Caciolli, A., Campostrini, M., Cavanna, F., Casaburo, F., Ciani, G. F., Colombetti, P., ... Viviani, M. (2024). Novel approach to infer the 2H⁡(𝑝,𝛾)⁢3He angular distribution: Experimental results and comparison with theoretical calculations. Physical Review C, 110(3), 1-7. Article L032801. https://doi.org/10.1103/PhysRevC.110.L032801

@article{9011fdf7f7904dfc882c1cf6ef72fee3,

title = "Novel approach to infer the 2H⁡(𝑝,𝛾)⁢3He angular distribution: Experimental results and comparison with theoretical calculations",

abstract = "The D(p,γ)3He reaction is of primary importance in cosmology and nuclear physics since it offers a unique opportunity to test predictions based on the description of nuclear interactions. We present a novel approach to extract the angular distribution of the photons emitted by the D(p,γ)3He reaction inferred from the shape of the experimental γ-spectra. The measurement was performed in the Gran Sasso Laboratories by the LUNA collaboration. By using a HPGe detector faced to an extended deuterium gas target, it was possible to derive the angular distribution in the 30-280 keV kinetic energy range and to compare the results with recent ab-initio predictions.",

author = "K Stockel and N. Mozumdar and S Zavatarelli and F Ferraro and M. Aliotta and C. Ananna and L. Barbieri and F Barile and D Bemmerer and A Best and A Boeltzig and C Broggini and Bruno, {C. G.} and A Caciolli and M. Campostrini and F Cavanna and F. Casaburo and Ciani, {G F} and P Colombetti and A. Compagnucci and P Corvisiero and L. Csedreki and T. Davinson and R Depalo and D. Dell'Aquila and {Di Leva}, A and Z Elekes and A Formicola and Zs Fulop and G Gervino and R Gesue and A Guglielmetti and C Gustavino and Gy Gyurky and A. Kievsky and G Imbriani and M Junker and M Lugaro and Marcucci, {L. E.} and P Marigo and J. Marsh and E Masha and R Menegazzo and D Mercogliano and V Mossa and V Paticchio and D Piatti and P Prati and D. Rapagnani and V. Rigato and D. Robb and L Schiavulli and R.S. Sidhu and J. Skowronski and O Straniero and T Szucs and M. Viviani",

year = "2024",

month = sep,

day = "18",

doi = "10.1103/PhysRevC.110.L032801",

language = "English",

volume = "110",

pages = "1--7",

journal = "Physical Review C",

issn = "2469-9985",

publisher = "American Physical Society",

number = "3",

}

Stockel, K, Mozumdar, N, Zavatarelli, S, Ferraro, F, Aliotta, M, Ananna, C, Barbieri, L, Barile, F, Bemmerer, D, Best, A, Boeltzig, A, Broggini, C, Bruno, CG, Caciolli, A, Campostrini, M, Cavanna, F, Casaburo, F, Ciani, GF, Colombetti, P, Compagnucci, A, Corvisiero, P, Csedreki, L, Davinson, T, Depalo, R, Dell'Aquila, D, Di Leva, A, Elekes, Z, Formicola, A, Fulop, Z, Gervino, G, Gesue, R, Guglielmetti, A, Gustavino, C, Gyurky, G, Kievsky, A, Imbriani, G, Junker, M, Lugaro, M, Marcucci, LE, Marigo, P, Marsh, J, Masha, E, Menegazzo, R, Mercogliano, D, Mossa, V, Paticchio, V, Piatti, D, Prati, P, Rapagnani, D, Rigato, V, Robb, D, Schiavulli, L, Sidhu, RS, Skowronski, J, Straniero, O, Szucs, T & Viviani, M 2024, 'Novel approach to infer the 2H⁡(𝑝,𝛾)⁢3He angular distribution: Experimental results and comparison with theoretical calculations', Physical Review C, vol. 110, no. 3, L032801, pp. 1-7. https://doi.org/10.1103/PhysRevC.110.L032801

TY - JOUR

T1 - Novel approach to infer the 2H⁡(𝑝,𝛾)⁢3He angular distribution: Experimental results and comparison with theoretical calculations

AU - Stockel, K

AU - Mozumdar, N.

AU - Zavatarelli, S

AU - Ferraro, F

AU - Aliotta, M.

AU - Ananna, C.

AU - Barbieri, L.

AU - Barile, F

AU - Bemmerer, D

AU - Best, A

AU - Boeltzig, A

AU - Broggini, C

AU - Bruno, C. G.

AU - Caciolli, A

AU - Campostrini, M.

AU - Cavanna, F

AU - Casaburo, F.

AU - Ciani, G F

AU - Colombetti, P

AU - Compagnucci, A.

AU - Corvisiero, P

AU - Csedreki, L.

AU - Davinson, T.

AU - Depalo, R

AU - Dell'Aquila, D.

AU - Di Leva, A

AU - Elekes, Z

AU - Formicola, A

AU - Fulop, Zs

AU - Gervino, G

AU - Gesue, R

AU - Guglielmetti, A

AU - Gustavino, C

AU - Gyurky, Gy

AU - Kievsky, A.

AU - Imbriani, G

AU - Junker, M

AU - Lugaro, M

AU - Marcucci, L. E.

AU - Marigo, P

AU - Marsh, J.

AU - Masha, E

AU - Menegazzo, R

AU - Mercogliano, D

AU - Mossa, V

AU - Paticchio, V

AU - Piatti, D

AU - Prati, P

AU - Rapagnani, D.

AU - Rigato, V.

AU - Robb, D.

AU - Schiavulli, L

AU - Sidhu, R.S.

AU - Skowronski, J.

AU - Straniero, O

AU - Szucs, T

AU - Viviani, M.

PY - 2024/9/18

Y1 - 2024/9/18

N2 - The D(p,γ)3He reaction is of primary importance in cosmology and nuclear physics since it offers a unique opportunity to test predictions based on the description of nuclear interactions. We present a novel approach to extract the angular distribution of the photons emitted by the D(p,γ)3He reaction inferred from the shape of the experimental γ-spectra. The measurement was performed in the Gran Sasso Laboratories by the LUNA collaboration. By using a HPGe detector faced to an extended deuterium gas target, it was possible to derive the angular distribution in the 30-280 keV kinetic energy range and to compare the results with recent ab-initio predictions.

AB - The D(p,γ)3He reaction is of primary importance in cosmology and nuclear physics since it offers a unique opportunity to test predictions based on the description of nuclear interactions. We present a novel approach to extract the angular distribution of the photons emitted by the D(p,γ)3He reaction inferred from the shape of the experimental γ-spectra. The measurement was performed in the Gran Sasso Laboratories by the LUNA collaboration. By using a HPGe detector faced to an extended deuterium gas target, it was possible to derive the angular distribution in the 30-280 keV kinetic energy range and to compare the results with recent ab-initio predictions.

U2 - 10.1103/PhysRevC.110.L032801

DO - 10.1103/PhysRevC.110.L032801

M3 - Letter

SN - 2469-9985

VL - 110

SP - 1

EP - 7

JO - Physical Review C

JF - Physical Review C

IS - 3

M1 - L032801

ER -

Novel approach to infer the 2H⁡(𝑝,𝛾)⁢3He angular distribution: Experimental results and comparison with theoretical calculations

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Edinburgh Nuclear Physics Group Consolidated Grant Proposal

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