Zobrazeno 1 - 10
of 10
pro vyhledávání: '"Ashabari Majumdar"'
Autor:
Jordan M. Roach, Khachatur V. Manukyan, Ashabari Majumdar, Stefania Dede, Allen G. Oliver, Peter C. Burns, Ani Aprahamian
Publikováno v:
Inorganic Chemistry. 60:18938-18949
Uranium dioxide (UO
Autor:
Jordan M Roach, Khachatur V. Manukyan, Peter C. Burns, Ani Aprahamian, Ashabari Majumdar, Daniel Robertson, Stefania Dede
Publikováno v:
ACS Applied Materials & Interfaces. 13:35153-35164
Combustion synthesis in uranyl nitrate-acetylacetone-2-methoxyethanol solutions was used to deposit thin UO2 films on aluminum substrates to investigate the irradiation-induced restructuring processes. Thermal analysis revealed that the combustion re
Autor:
Ashabari Majumdar, Khachatur V. Manukyan, Wanpeng Tan, Stefania Dede, Jordan M. Roach, Aaron Couture, Peter C. Burns, Ani Aprahamian
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 1045:167551
Autor:
Graham F. Peaslee, Khachatur V. Manukyan, Edward Stech, Mark Raddell, Michael Wiescher, Cecilia Fasano, Ashabari Majumdar
Publikováno v:
Applied Surface Science. 493:818-828
This work presents results of macro, micro, and nanoscale surface characterization for a set of Roman denarii, ranging from 136 BCE to 240 CE, using large-scale X-ray fluorescence (XRF) mapping, particle-induced X-ray emission (PIXE) spectroscopy, fo
Autor:
Stefania Dede, Khachatur V. Manukyan, Jordan M. Roach, Ashabari Majumdar, Peter C. Burns, Ani Aprahamian
Publikováno v:
Applied Surface Science. 603:154437
Autor:
Ashabari, Majumdar, Khachatur V, Manukyan, Stefania, Dede, Jordan M, Roach, Daniel, Robertson, Peter C, Burns, Ani, Aprahamian
Publikováno v:
ACS applied materialsinterfaces. 13(29)
Combustion synthesis in uranyl nitrate-acetylacetone-2-methoxyethanol solutions was used to deposit thin UO
Autor:
Rebeka Kelmar, Stefan Typel, D. Lattuada, M. S. Kwag, Wanpeng Tan, D. Blankstein, V. Burjan, L. Boccioli, Roberta Spartà, S. Anguilar, M. R. Hall, J. Long, A. Gula, A. A. Oliva, A. Tumino, J. Mrazek, M. La Commara, C. Spitaleri, Patrick O'Malley, B. Frentz, G. D’Agata, G. G. Rapisarda, S. L. Henderson, S. Romano, Lauren Callahan, A. M. Clark, M. L. Sergi, G. L. Guardo, M. Mazzocco, D. W. Bardayan, Michael Wiescher, Sara Palmerini, Michael Skulski, K. Y. Chae, I. Indelicato, Manoel Couder, P. M. Prajapati, Austin Nelson, M. La Cognata, Sean R. McGuinness, S. M. Cha, Q. Liu, Livio Lamia, C. Spampinato, R. G. Pizzone, John Wilkinson, Christopher Seymour, Ashabari Majumdar
Publikováno v:
The European Physical Journal A. 56
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 that drove the elemental nucleosynthesis in the first 20 min of the history of the Universe.
Autor:
K. T. Macon, Patrick O'Malley, D. W. Bardayan, B. Vande Kolk, S. Moylan, K. L. Jones, Richard deBoer, Jerome Kovoor, S. Jin, Maxime Renaud, Khachatur V. Manukyan, K. Y. Chae, Tan Ahn, A. Boeltzig, Michael Wiescher, Karl Smith, Carl R. Brune, Wanpeng Tan, S. L. Henderson, Sebastian Aguilar, L. Morales, Shea Mosby, S. Burcher, Ashabari Majumdar
Publikováno v:
Proceedings of the 15th International Symposium on Origin of Matter and Evolution of Galaxies (OMEG15).
Autor:
D. Blankstein, Lauren Callahan, G. G. Rapisarda, C. Seyymour, Livio Lamia, G. L. Guardo, C. Spampinato, D. Bardyan, M. L. Sergi, L. Boccioli, Manoel Couder, Roberta Spartà, P. M. Prajapati, A. M. Clark, V. Burian, Austin Nelson, Sean R. McGuinness, G. D’Agata, A. Tumino, M. La Cognata, Michael Skulski, K. Y. Chae, J. Long, Q. Liu, Ashabari Majumdar, Rebeka Kelmar, C. Spitaleri, John Wilkinson, S. Romano, A. A. Oliva, Patrick O'Malley, S. L. Henderson, J. Mrazek, R. G. Pizzone, I. Indelicato, D. Lattuada, Michael Wiescher, M. R. Hall, A. Gula, B. Frentz, S. Anguilar, W. Tan, Sara Palmerini
Publikováno v:
EPJ Web of Conferences, Vol 227, p 02013 (2020)
In the network of reactions present in the Big Bang nucleosynthesis, the 3He(n, p)3H has an important role which impacts the final 7Li abundance. The Trojan Horse Method (THM) has been applied to the 3He(d, pt)H reaction in order to extract the astro
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0fbb0cc3430c9d6a571f13f8c29966a9
http://hdl.handle.net/11391/1490612
http://hdl.handle.net/11391/1490612
Autor:
D. Blankstein, Q. Liu, S. Anguilar, W. Tan, M. L. Sergi, G. D’Agata, D. Lattuada, J. Mrazek, Rebeka Kelmar, Sara Palmerini, Christopher Seymour, Lauren Callahan, John Wilkinson, A. M. Clark, A. A. Oliva, Patrick O'Malley, Ashabari Majumdar, Livio Lamia, R. G. Pizzone, V. Burian, Sean R. McGuinness, C. Spampinato, G. L. Guardo, L. Boccioli, D. W. Bardayan, Michael Wiescher, S. L. Henderson, G. G. Rapisarda, M. La Cognata, Claudio Spitaleri, P. M. Prajapati, Austin Nelson, M. R. Hall, A. Gula, B. Frentz, A. Tumino, S. Romano, Manoel Couder, J. Long, Michael Skulski, K. Y. Chae
Publikováno v:
Journal of Physics: Conference Series. 1668:012039
In the network of reactions present in the Big Bang nucleosynthesis, the 3He(n, p)3H reaction has an important role which impacts the final 7Li abundance. The Trojan Horse Method (THM) has been applied to the 3He(d, pt)H reaction in order to extract