Search Results - "Prajapati P. M."

A New Reaction Rate of the 27Al(p/α)24Mg Reaction Based on Indirect Measurements at Astrophysical Energies and Implications for 27Al Yields of Intermediate-mass Stars by La Cognata, M., Palmerini, S., Adsley, P., Hammache, F., Di Pietro, A., Figuera, P., Dell’Agli, F., Alba, R., Cherubini, S., Guardo, G. L., Gulino, M., Lamia, L., Lattuada, D., Maiolino, C., Oliva, A., Pizzone, R. G., Prajapati, P. M., Rapisarda, G. G., Romano, S., Santonocito, D., Spartá, R., Sergi, M. L., Tumino, A., Ventura, P.

“…The abundance of 26Al carries a special role in astrophysics, since it probes active nucleosynthesis in the Milky Way and constrains the Galactic core-collapse…”
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Indirect measurement of the $$^3\hbox {He}$$(n,p)$$^3\hbox {H}$$ reaction cross section at Big Bang energies by Pizzone, R. G., Spampinato, C., Spartá, R., Couder, M., Tan, W., Burjan, V., D’Agata, G., Guardo, G. L., La Cognata, M., Lamia, L., Mrazek, J., Palmerini, S., Typel, S., Tumino, A., Wiescher, M., Anguilar, S., Bardayan, D., Blankstein, D., Boccioli, L., Callahan, L., Cha, S. M., Chae, K. Y., Clark, A. M., Frentz, B., Hall, M. R., Gula, A., Henderson, S., Kelmar, R., Kwag, M. S., Indelicato, I., La Commara, M., Lattuada, D., Liu, Q., Long, J., Mazzocco, M., Majumdar, A., McGuinness, S., Nelson, A., Oliva, A. A., O’Malley, P., Prajapati, P. M., Rapisarda, G. G., Romano, S., Sergi, M. L., Seymour, C., Skulski, M., Spitaleri, C., Wilkinson, J.

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Indirect measurement of the 3He(n,p)3H reaction cross section at Big Bang energies by Pizzone, R. G., Spampinato, C., Spartá, R., Couder, M., Tan, W., Burjan, V., D’Agata, G., Guardo, G. L., La Cognata, M., Lamia, L., Mrazek, J., Palmerini, S., Typel, S., Tumino, A., Wiescher, M., Anguilar, S., Bardayan, D., Blankstein, D., Boccioli, L., Callahan, L., Cha, S. M., Chae, K. Y., Clark, A. M., Frentz, B., Hall, M. R., Gula, A., Henderson, S., Kelmar, R., Kwag, M. S., Indelicato, I., La Commara, M., Lattuada, D., Liu, Q., Long, J., Mazzocco, M., Majumdar, A., McGuinness, S., Nelson, A., Oliva, A. A., O’Malley, P., Prajapati, P. M., Rapisarda, G. G., Romano, S., Sergi, M. L., Seymour, C., Skulski, M., Spitaleri, C., Wilkinson, J.

“…Nuclear reactions play a key role in the framework of the Big Bang Nucleosynthesis. A network of 12 principal reactions has been identified as the main path…”
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Scattering chamber facility for double-differential cross-section measurement with 14 MeV DT neutron generator at IPR by PRAJAPATI, P M, PANDEY, BHAWNA, GUPTA, N C, KUMAR, SURESH, NAYAK, B K, SAXENA, A, SURYANARAYANA, S V, JAKHAR, S, VALA, SUDHIRSINH, RAO, C V S, BASU, T K

“…Measurement of double-differential cross-sections of 14 MeV neutron-induced charged-particle productions is very important for estimating the nuclear heating…”
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Measurement of 56Fe(n, p)56Mn reaction cross-section at E n = 5.9, 9.85, 14.8 and 15.5 MeV by Mulik, V. K., Naik, H., Suryanarayana, S. V., Dhole, S. D., Prajapati, P. M., Shivashankar, B. S., Jagadeesan, K. C., Thakre, S. V., Bhoraskar, V. N., Goswami, A.

“…The 56Fe(n, p)56Mn reaction cross-section at neutron energies of 5.9 A- 0.6, 9.85 A- 0.38, 14.8 A- 0.1 and 15.5 A- 0.7 MeV from the 7Li(p, n) as well as 3H(d,…”
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Photo-neutron cross-section of 100Mo by Crasta, Rita, Naik, H., Suryanarayana, S. V., Prajapati, P. M., Jagadisan, K. C., Thakare, S. V., Ganesh, S., Nimje, V. T., Mittal, K. C., Goswami, A.

“…The 100 Mo(γ, n) reaction cross-section was experimentally determined at end point bremsstrahlung energy of 10 and 12.5 MeV using off-line γ-ray spectrometric…”
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Measurement of flux distribution of an AmBe neutron source and estimation of two group integral capture cross-sections by Guruprasad, Shet, Sachin, Prajapati, P.M., Suryanarayana, S.V., Karkera, Meghna, Subbaiah, K.V., Raviprakash, Y., Shivashankar, B.S.

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Validation of MCkeff code using ICSBEP results by Shet, Sachin, Subbaiah, K.V., Prajapati, P.M., Singh, Kapil Deo, Anand, S., Suryanarayna, S.V.

“…Validation of the indigenously developed Monte Carlo program, MCkeff, is carried out by comparing the results of International Criticality Safety Benchmark…”
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A New Reaction Rate of the $^{27}$Al(p/α)$^{24}$Mg Reaction Based on Indirect Measurements at Astrophysical Energies and Implications for $^{27}$Al Yields of Intermediate-mass Stars by La Cognata, M., Palmerini, S., Adsley, P., Hammache, F., Di Pietro, A., Figuera, P., Dell’agli, F., Alba, R., Cherubini, S., Guardo, G.L., Gulino, M., Lamia, L., Lattuada, D., Maiolino, C., Oliva, A., Pizzone, R.G., Prajapati, P.M., Rapisarda, G.G., Romano, S., Santonocito, D., Spartá, R., Sergi, M.L., Tumino, A., Ventura, P.

“…The abundance of $^{26}$Al carries a special role in astrophysics, since it probes active nucleosynthesis in the Milky Way and constrains the Galactic…”
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A New Reaction Rate of the 27 Al(p/α) 24 Mg Reaction Based on Indirect Measurements at Astrophysical Energies and Implications for 27 Al Yields of Intermediate-mass Stars by La Cognata, M., Palmerini, S., Adsley, P., Hammache, F., Di Pietro, A., Figuera, P., Dell’Agli, F., Alba, R., Cherubini, S., Guardo, G. L., Gulino, M., Lamia, L., Lattuada, D., Maiolino, C., Oliva, A., Pizzone, R. G., Prajapati, P. M., Rapisarda, G. G., Romano, S., Santonocito, D., Spartá, R., Sergi, M. L., Tumino, A., Ventura, P.

“…The abundance of 26 Al carries a special role in astrophysics, since it probes active nucleosynthesis in the Milky Way and constrains the Galactic…”
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Indirect Measurement of the 3 He(n,p) 3 H Reaction Cross Section at Big Bang Energies by Pizzone, R. G., Sergi, M. L., Oliva, A. A., Zanatta-Martinez, T., Lamia, L., Spartá, R., Guardo, G. L., La Cognata, M., D’Agata, G., Palmerini, S., Tumino, A., Costa, M., Cittadino, D., Di Pietro, A., Figuera, P., Indelicato, I., Massara, A., Cherubini, S., Rapisarda, G. G., Romano, S., Spampinato, C., Couder, M., Tan, W., Wiescher, M., Lattuada, D., Gulino, M., Burjan, V., Mrazek, J., La Commara, M., Mazzocco, M., Prajapati, P. M., Aguilar, S., Anderson, T., Bardayan, D., Blankstein, D., Callahan, L., Clark, A., Frentz, B., Gula, A., Hall, M., Henderson, S. L., Kelmar, R., Liu, Q., Long, J., Majundar, A., McGiunness, S., Nelson, A., O’Malley, P., Seimour, C., Skulski, M., Wilkinson, J., Cha, S. M., Chae, K. Y., Kwag, M. S., Typel, S.

“…Neutron-induced nuclear reactions play an important role in the Big Bang Nucleosynthesis. Their excitation functions are, from an experimental point of view,…”
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Production and characterisation of 20,22Ne targets by Prajapati, P M, Pizzone, R G, Hingu, Akash, Mukherjee, S, Suryanarayana, S V

“…Targets of 20 Ne and 22 Ne nuclides were produced for nuclear astrophysics experiments by implanting them into tantalum backing material at the Ion Beam Centre…”
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Indirect Measurement of the 3He(n,p)3H Reaction Cross Section at Big Bang Energies by Pizzone, R. G., Sergi, M. L., Oliva, A. A., Zanatta-Martinez, T., Lamia, L., Spartá, R., Guardo, G. L., La Cognata, M., D’Agata, G., Palmerini, S., Tumino, A., Costa, M., Cittadino, D., Di Pietro, A., Figuera, P., Indelicato, I., Massara, A., Cherubini, S., Rapisarda, G. G., Romano, S., Spampinato, C., Couder, M., Tan, W., Wiescher, M., Lattuada, D., Gulino, M., Burjan, V., Mrazek, J., La Commara, M., Mazzocco, M., Prajapati, P. M., Aguilar, S., Anderson, T., Bardayan, D., Blankstein, D., Callahan, L., Clark, A., Frentz, B., Gula, A., Hall, M., Henderson, S. L., Kelmar, R., Liu, Q., Long, J., Majundar, A., McGiunness, S., Nelson, A., O’Malley, P., Seimour, C., Skulski, M., Wilkinson, J., Cha, S. M., Chae, K. Y., Kwag, M. S., Typel, S.

“…Neutron-induced nuclear reactions play an important role in the Big Bang Nucleosynthesis. Their excitation functions are, from an experimental point of view,…”
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Physical and acoustical properties of paracetamol in binary mixtures of water + propylene glycol by Prajapati, P.M., Pandit, T.R., Vankar, H.P., Rana, V.A.

“…Experimental results of physical properties (density, viscosity and refractive index) and acoustical property (speed of sound) for a range of concentrations of…”
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Study of the 12 C + 16 O fusion reaction in carbon burning via the Trojan Horse Method by Oliva, A. A., Tumino, A., Soic, N., Prajapati, P. M., Acosta, L., Alba, R., Barba, F., Cherubini, S., D’Agata, G., Dell’Aquila, D., Di Pietro, A., Fernandez, J.P., Figuera, P., Galaviz Redondo, D., Guardo, L., Gulino, M., Hammache, F., Jelavic Malenica, D., Kiliç, A.I., La Cognata, M., La Commara, M., Lamia, L., Lattuada, D., Maiolino, C., Manicò, G., Mazzocco, M., Milin, M., Nanru, Ma, Nurmukhanbetova, A., Nurkic, D., Palmerini, S., Parascandolo, T., Pierroutsakou, D., Pizzone, R.G., Popocovski, R., Rapisarda, G.G., Romano, S., Santonocito, D., Sergi, M.L., Shotter, A., Spartà, R., Spiridon, A., Trache, L., Vukman, N., Yamaguchi, H.

“…12 C + 12 C is the main reaction during core and shell carbon burning in massive stars, however, at temperatures higher than 10 9 K when most of the carbon is…”
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Study of the 12C +16 O fusion reaction in carbon burning via the Trojan Horse Method by Oliva A. A., Tumino A., Soic N., Prajapati P. M., Acosta L., Alba R., Barba F., Cherubini S., D’Agata G., Dell’Aquila D., Di Pietro A., Fernandez J.P., Figuera P., Galaviz Redondo D., Guardo L., Gulino M., Hammache F., Jelavic Malenica D., Kiliç A.I., La Cognata M., La Commara M., Lamia L., Lattuada D., Maiolino C., Manicò G., Mazzocco M., Milin M., Nanru Ma, Nurmukhanbetova A., Nurkic D., Palmerini S., Parascandolo T., Pierroutsakou D., Pizzone R.G., Popocovski R., Rapisarda G.G., Romano S., Santonocito D., Sergi M.L., Shotter A., Spartà R., Spiridon A., Trache L., Vukman N., Yamaguchi H.

“…12C +12 C is the main reaction during core and shell carbon burning in massive stars, however, at temperatures higher than 109K when most of the carbon is…”
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Mass distribution in the quasi-mono-energetic neutron-induced fission of 232Th by Naik, H., Crasta, Rita, Suryanarayana, S. V., Prajapati, P. M., Mulik, V. K., Shivasankar, B. S., Jagadeesan, K. C., Thakare, S. V., Sharma, S. C., Goswami, A.

“… The cumulative yields of various fission products in 232 Th(n, f) with average neutron energies of 6.35, 8.53 and 10.09 MeV have been determined using an…”
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Measurement of the neutron capture cross-section of [sup.238]U using the neutron activation technique by Naik, H, Surayanarayana, S.V, Mulik, V.K, Prajapati, P.M, Shivashankar, B.S, Jagadeesan, K.C, Thakare, S.V, Raj, D, Sharma, S.C, Bhagwat, P.V, Dhole, S.D, Ganesan, S, Bhoraskar, V.N, Goswami, A

“…The [sup.238]U(n, γ)[sup.239]U reaction cross-section at average neutron energy of 3.7 ± 0.3 MeV from the [sup.7]Li(p, n)[sup.7]Be reaction has been determined…”
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Measurement of 56Fe(n, p)56Mn reaction cross-section at En = 5.9, 9.85, 14.8 and 15.5 MeV by Mulik, V. K., Naik, H., Suryanarayana, S. V., Dhole, S. D., Prajapati, P. M., Shivashankar, B. S., Jagadeesan, K. C., Thakre, S. V., Bhoraskar, V. N., Goswami, A.

“…The 56 Fe(n, p) 56 Mn reaction cross-section at neutron energies of 5.9 ± 0.6, 9.85 ± 0.38, 14.8 ± 0.1 and 15.5 ± 0.7 MeV from the 7 Li(p, n) as well as 3 H(d,…”
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Measurement of the neutron capture cross-sections of 232Th at 5.9 MeV and 15.5 MeV by Prajapati, P. M., Naik, H., Suryanarayana, S. V., Mukherjee, S., Jagadeesan, K. C., Sharma, S. C., Thakre, S. V., Rasheed, K. K., Ganesan, S., Goswami, A.

“… The 232 Th(n, γ) 233 Th reaction cross-section has been determined for the first time using an activation and off-line γ-ray spectrometric technique at…”
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