First Direct Measurement of Mg(α,p)25Al and Implications for X-Ray Burst Model-Observation Comparisons
Abstract
Type-I x-ray bursts can reveal the properties of an accreting neutron star system when compared with astrophysics model calculations. However, model results are sensitive to a handful of uncertain nuclear reaction rates, such as 22Mg(α , p). We report the first direct measurement of 22Mg(α , p), performed with the Active Target Time Projection Chamber. The corresponding astrophysical reaction rate is orders of magnitude larger than determined from a previous indirect measurement in a broad temperature range. Overall, our new measurement suggests a less-compact neutron star in the source GS1826-24.
- Authors:
-
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- Michigan State Univ., East Lansing, MI (United States). National Superconducting Cyclotron Lab.; Joint Inst. for Nuclear Astrophysics (JINA), East Lansing, MI (United States). Center for the Evolution of the Elements (JINA-CEE)
- Michigan State Univ., East Lansing, MI (United States). National Superconducting Cyclotron Lab.
- Michigan State Univ., East Lansing, MI (United States). National Superconducting Cyclotron Lab.; Michigan State Univ., East Lansing, MI (United States)
- Ohio Univ., Athens, OH (United States). Inst. of Nuclear and Particle Physics
- Univ. of Notre Dame, IN (United States)
- Univ. Santiago de Compostela (Spain). IGFAE
- Michigan State Univ., East Lansing, MI (United States)
- Joint Inst. for Nuclear Astrophysics (JINA), East Lansing, MI (United States). Center for the Evolution of the Elements (JINA-CEE); Central Michigan Univ., Mount Pleasant, MI (United States)
- Michigan State Univ., East Lansing, MI (United States). National Superconducting Cyclotron Lab.; Ruđer Bošković Inst., Zagreb (Croatia)
- Michigan State Univ., East Lansing, MI (United States). National Superconducting Cyclotron Lab.; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Michigan State Univ., East Lansing, MI (United States). National Superconducting Cyclotron Lab.; Joint Inst. for Nuclear Astrophysics (JINA), East Lansing, MI (United States). Center for the Evolution of the Elements (JINA-CEE); Michigan State Univ., East Lansing, MI (United States)
- Michigan State Univ., East Lansing, MI (United States). National Superconducting Cyclotron Lab.; Univ. de Sao Paulo (Brazil). Inst. de Fisica
- Publication Date:
- Research Org.:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC), Nuclear Physics (NP); National Science Foundation (NSF); FAPESP
- OSTI Identifier:
- 1823254
- Grant/Contract Number:
- AC02-05CH11231; MRI-0923087; PHY-140444; PHY-1565546; PHY-1713857; PHY-1430152; PHY-1102511; PHY-1913554; 14-01343; FG02-88ER40387; SC0019042; 2018/04965-4
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Physical Review Letters
- Additional Journal Information:
- Journal Volume: 125; Journal Issue: 20; Journal ID: ISSN 0031-9007
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 73 NUCLEAR PHYSICS AND RADIATION PHYSICS; nuclear astrophysics; nuclear physics of explosive environments; nuclear reactions
Citation Formats
Randhawa, J. S., Ayyad, Y., Mittig, W., Meisel, Z., Ahn, T., Aguilar, S., Alvarez-Pol, H., Bardayan, D. W., Bazin, D., Beceiro-Novo, S., Blankstein, D., Carpenter, L., Cortesi, M., Cortina-Gil, D., Gastis, P., Hall, M., Henderson, S., Kolata, J. J., Mijatovic, T., Ndayisabye, F., O’Malley, P., Pereira, J., Pierre, A., Robert, H., Santamaria, C., Schatz, H., Smith, J., Watwood, N., and Zamora, J. C. First Direct Measurement of Mg(α,p)25Al and Implications for X-Ray Burst Model-Observation Comparisons. United States: N. p., 2020.
Web. doi:10.1103/physrevlett.125.202701.
Randhawa, J. S., Ayyad, Y., Mittig, W., Meisel, Z., Ahn, T., Aguilar, S., Alvarez-Pol, H., Bardayan, D. W., Bazin, D., Beceiro-Novo, S., Blankstein, D., Carpenter, L., Cortesi, M., Cortina-Gil, D., Gastis, P., Hall, M., Henderson, S., Kolata, J. J., Mijatovic, T., Ndayisabye, F., O’Malley, P., Pereira, J., Pierre, A., Robert, H., Santamaria, C., Schatz, H., Smith, J., Watwood, N., & Zamora, J. C. First Direct Measurement of Mg(α,p)25Al and Implications for X-Ray Burst Model-Observation Comparisons. United States. https://doi.org/10.1103/physrevlett.125.202701
Randhawa, J. S., Ayyad, Y., Mittig, W., Meisel, Z., Ahn, T., Aguilar, S., Alvarez-Pol, H., Bardayan, D. W., Bazin, D., Beceiro-Novo, S., Blankstein, D., Carpenter, L., Cortesi, M., Cortina-Gil, D., Gastis, P., Hall, M., Henderson, S., Kolata, J. J., Mijatovic, T., Ndayisabye, F., O’Malley, P., Pereira, J., Pierre, A., Robert, H., Santamaria, C., Schatz, H., Smith, J., Watwood, N., and Zamora, J. C. Tue .
"First Direct Measurement of Mg(α,p)25Al and Implications for X-Ray Burst Model-Observation Comparisons". United States. https://doi.org/10.1103/physrevlett.125.202701. https://www.osti.gov/servlets/purl/1823254.
@article{osti_1823254,
title = {First Direct Measurement of Mg(α,p)25Al and Implications for X-Ray Burst Model-Observation Comparisons},
author = {Randhawa, J. S. and Ayyad, Y. and Mittig, W. and Meisel, Z. and Ahn, T. and Aguilar, S. and Alvarez-Pol, H. and Bardayan, D. W. and Bazin, D. and Beceiro-Novo, S. and Blankstein, D. and Carpenter, L. and Cortesi, M. and Cortina-Gil, D. and Gastis, P. and Hall, M. and Henderson, S. and Kolata, J. J. and Mijatovic, T. and Ndayisabye, F. and O’Malley, P. and Pereira, J. and Pierre, A. and Robert, H. and Santamaria, C. and Schatz, H. and Smith, J. and Watwood, N. and Zamora, J. C.},
abstractNote = {Type-I x-ray bursts can reveal the properties of an accreting neutron star system when compared with astrophysics model calculations. However, model results are sensitive to a handful of uncertain nuclear reaction rates, such as 22Mg(α , p). We report the first direct measurement of 22Mg(α , p), performed with the Active Target Time Projection Chamber. The corresponding astrophysical reaction rate is orders of magnitude larger than determined from a previous indirect measurement in a broad temperature range. Overall, our new measurement suggests a less-compact neutron star in the source GS1826-24.},
doi = {10.1103/physrevlett.125.202701},
journal = {Physical Review Letters},
number = 20,
volume = 125,
place = {United States},
year = {Tue Nov 10 00:00:00 EST 2020},
month = {Tue Nov 10 00:00:00 EST 2020}
}
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