B. Schmidt - List of publications at the Cyclotron Institute, Texas A&M University

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Cannot merge authors: insufficient rights.

First name(s):	B.
Last name(s):	Schmidt

Authors associated with the Cyclotron Institute are underlined, and those associated with Center of Excellence in Nuclear Training And University-based Research (CENTAUR) have a ^* next to their name.

Determination of the astrophysical factor of the $^3\mathrm{He}(\alpha,\gamma)^7\mathrm{Be}$ down to zero energy using the asymptotic normalization coefficient method, M. La Cognata, G. G. Kiss, R. Yarmukhamedov, K. I. Tursunmakhatov, I. Wiedenhöver^*, L. T. Baby, S. Cherubini, A. Cvetinović, G. D'Agata, P. Figuera, G. L. Guardo, M. Gulino, S. Hayakawa, I. Indelicato, L. Lamia, M. Lattuada, F. Mudò, S. Palmerini, R. G. Pizzone, G. G. Rapisarda, S. Romano, M. L. Sergi, R. Spartá, C. Spitaleri, O. Trippella, A. Tumino, M. Anastasiou, S. A. Kuvin, N. Rijal, B. Schmidt, S. B. Igamov, S. B. Sakuta, Zs. Fülöp, Gy. Gyürky, T. Szücs, Z. Halász, E. Somorjai, Z. Hons, J. Mrazek, R. E. Tribble and A. M. Mukhamedzhanov^*, in: 28th International Nuclear Physics Conference (INPC 2022), Journal of Physics: Conference Series 2586, Cape Town South Africa, pages 012093, {IOP} Publishing, 2023

pub id: 1337 [DOI] [URL]

Astrophysical $S$-factor for the $^3\mathrm{He}(\alpha,\gamma)^7\mathrm{Be}$ reaction via the asymptotic normalization coefficient ({ANC}) method, G. G. Kiss, M. La Cognata, C. Spitaleri, R. Yarmukhamedov, I. Wiedenhöver^*, L. T. Baby, S. Cherubini, A. Cvetinović, G. D'Agata, P. Figuera, G. L. Guardo, M. Gulino, S. Hayakawa, I. Indelicato, L. Lamia, M. Lattuada, F. Mudò, S. Palmerini, R. G. Pizzone, G. G. Rapisarda, S. Romano, M. L. Sergi, R. Spartá, O. Trippella, A. Tumino, M. Anastasiou, S. A. Kuvin, N. Rijal, B. Schmidt, S. B. Igamov, S. B. Sakuta, K. I. Tursunmakhatov, Zs. Fülöp, Gy. Gyürky, T. Szücs, Z. Halász, E. Somorjai, Z. Hons, J. Mrazek, R. E. Tribble and A. M. Mukhamedzhanov^*, Physics Letters B 807, 135606 (2020)

pub id: 1040 [DOI] [URL]

Indirect determination of the astrophysical $S$ factor for the $^6\mathrm{Li}(p,\gamma)^7\mathrm{Be}$ reaction using the asymptotic normalization coefficient method, G. G. Kiss, M. La Cognata, R. Yarmukhamedov, K. I. Tursunmakhatov, I. Wiedenhöver^*, L. T. Baby, S. Cherubini, A. Cvetinović, G. D'Agata, P. Figuera, G. L. Guardo, M. Gulino, S. Hayakawa, I. Indelicato, L. Lamia, M. Lattuada, F. Mudò, S. Palmerini, R. G. Pizzone, G. G. Rapisarda, S. Romano, M. L. Sergi, R. Spartá, C. Spitaleri, O. Trippella, A. Tumino, M. Anastasiou, S. A. Kuvin, N. Rijal, B. Schmidt, S. B. Igamov, S. B. Sakuta, Zs. Fülöp, Gy. Gyürky, T. Szücs, Z. Halász, E. Somorjai, Z. Hons, J. Mrazek, R. E. Tribble and A. M. Mukhamedzhanov^*, Phys. Rev. C 104, 015807 (2021)

pub id: 1142 [DOI] [URL]

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