Cosmological Lithium Problems by Bertulani C.A., chintak Shubh, Mukhamedzhanov A.M.

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Surface-Integral Approach to the Coulomb Few-Body Scattering Problem by Stelbovics A.T., Mukhamedzhanov A.M., Bray I., Kadyrov A.S.

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Trojan Horse particle invariance for 2H(d,p)3H reaction: a detailed study by Pizzone R.G., Spitaleri C., Bertulani C.A., Mukhamedzhanov A.M., Blokhintsev L., La Cognata M., Lamia L., Rinollo A., Spartá R., Tumino A.

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The astrophysical S-factor of the direct 18O(p, γ)19F capture by the ANC method by Burjan V., Hons Z., Kroha V., Mrázek J., Piskoř Š., Mukhamedzhanov A. M., Trache L., Tribble R. E., La Cognata M., Lamia L., Pizzone G. R., Romano S., Spitaleri C., Tumino A.

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Measurement of sub threshold resonance contributions to fusion reactions: the case of the 13C(α, n)16O astrophysical neutron source by La Cognata M., Spitaleri C., Trippella O., Kiss G.G., Rogachev G.V., Mukhamedzhanov A.M., Avila M., Guardo G.L., Koshchiy E., Kuchera A., Lamia L., Puglia S.M.R., Romano S., Santiago D., Spartà R.

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ANC experiments for nuclear astrophysics in NPI CAS by Mrazek J., Burjan V., Kroha V., Mukhamedzhanov A.M., Tribble R., Spitaleri C., Siváček I., Glagolev V., Piskoř Š., Pizzone G.R., La Cognata M., D’Agata G., Tumino A., Lamia L., Sparta R., Rapisarda G., Romano S.

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Measurement of the 13C(α, n)16O reaction at astrophysical energies using the Trojan Horse Method. Focus on the -3 keV sub-threshold resonance by La Cognata M., Spitaleri C., Trippella O., Kiss G.G., Rogachev G.V., Mukhamedzhanov A.M., Avila M., Guardo G.L., Koshchiy E., Kuchera A., Lamia L., Puglia S.M.R., Romano S., Santiago D., Spartà R.

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Application of the Trojan Horse Method to study neutron induced reactions: the 17O(n, α)14C reaction by Gulino M., Spitaleri C., Tang X.D., Guardo G.L., Lamia L., Cherubini S., Bucher B., Burjan V., Couder M., Davies P., deBoer R., Fang X., Goldberg V.Z., Hons Z., Kroha V., Lamm L., La Cognata M., Li C., Ma C., Mrazek J., Mukhamedzhanov A.M., Notani M., O’Brien S., Pizzone R.G., Rapisarda G.G., Roberson D., Sergi M.L., Tan W., Thompson I.J., Wiescher M.

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Determination of the 3He(α, γ)7Be and 6Li(p, γ)7Be astrophysical factors down to zero energy using the asymptotic normalization coefficients by La Cognata M., Kiss G. G., Yarmukhamedov R., Tursunmakhatov K. I., Wiedenhöver I., Baby L. T., Cherubini S., Cvetinović A., D’Agata G., Figuera P., Guardo G.L., Gulino M., Hayakawa S., Indelicato I., Lamia L., Lattuada M., Mudò F., Palmerini S., Pizzone R.G., Rapisarda G.G., Romano S., Sergi M. L., Spartà R., Spitaleri C., Trippella O., Tumino A., Anastasiou M., Kuvin S. A., Rijal N., Schmidt B., Igamov S. B., Sakuta S. B., Fülöp Zs., Gyürky Gy., Szücs T., Halász Z., Somorjai E., Hons Z., Mrázek J., Tribble R. E., Mukhamedzhanov A. M.

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