Zobrazeno 1 - 10
of 786
pro vyhledávání: '"Barnes, JR"'
Autor:
BARNES JR, MELVIN1,2
Publikováno v:
Journal of World History. Sep2023, Vol. 34 Issue 3, p463-490. 28p.
Autor:
JEFFERSON, DAVID, BARNES JR., PETER D.
Publikováno v:
ACM Transactions on Modeling & Computer Simulation; Oct2024, Vol. 34 Issue 4, p1-35, 35p
Autor:
Paley, J. M., Messier, M. D., Raja, R., Akgun, U., Asner, D. M., Aydin, G., Baker, W., Barnes, Jr., P. D., Bergfeld, T., Beverly, L., Bhatnagar, V., Choudhary, B., Dukes, E. C., Duru, F., Feldman, G. J., Godley, A., Graf, N., Gronberg, J., Gulmez, E., Gunaydin, Y. O., Gustafson, H. R., Hartouni, E. P., Hanlet, P., Heffner, M., Kaplan, D. M., Kamaev, O., Klay, J., Kumar, A., Lange, D. J., Lebedev, A., Ling, J., Longo, M. J., Lu, L. C., Materniak, C., Mahajan, S., Meyer, H., Miller, D. E., Mishra, S. R., Nelson, K., Nigmanov, T., Norman, A., Onel, Y., Penzo, A., Peterson, R. J., Rajaram, D., Ratnikov, D., Rosenfeld, C., Rubin, H., Seun, S., Singh, A., Solomey, N., Soltz, R. A., Torun, Y., Wilson, K., Wright, D. M., Wu, Q. K.
Publikováno v:
Phys. Rev. D 90, 032001 (2014)
The fixed-target MIPP experiment, Fermilab E907, was designed to measure the production of hadrons from the collisions of hadrons of momenta ranging from 5 to 120 GeV/c on a variety of nuclei. These data will generally improve the simulation of parti
Externí odkaz:
http://arxiv.org/abs/1404.5882
Autor:
Nigmanov, T. S., Rajaram, D., Longo, M. J., Akgun, U., Aydin, G., Baker, W., Barnes, Jr., P. D., Bergfeld, T., Bujak, A., Carey, D., Dukes, E. C., Duru, F., Feldman, G. J., Godley, A., Gülmez, E., Günaydin, Y. O., Graf, N., Gustafson, H. R., Gutay, L., Hartouni, E., Hanlet, P., Heffner, M., Johnstone, C., Kaplan, D. M., Kamaev, O., Klay, J., Kostin, M., Lange, D., Lebedev, A., Lu, L. C., Materniak, C., Messier, M. D., Meyer, H., Miller, D. E., Mishra, S. R., Nelson, K. S., Norman, A., Onel, Y., Paley, J. M., Park, H. K., Penzo, A., Peterson, R. J., Raja, R., Rosenfeld, C., Rubin, H. A., Seun, S., Solomey, N., Soltz, R., Swallow, E., Torun, Y., Wilson, K., Wright, D., Wu, K.
Publikováno v:
Phys.Rev.D83:012002,2011
We have measured cross sections for forward neutron production from a variety of targets using proton beams from the Fermilab Main Injector. Measurements were performed for proton beam momenta of 58 GeV/c, 84 GeV/c, and 120 GeV/c. The cross section d
Externí odkaz:
http://arxiv.org/abs/1010.6291
Autor:
The MIPP Collaboration, Graf, N., Lebedev, A., Abrams, R. J., Akgun, U., Aydin, G., Baker, W., Barnes Jr., P. D., Bergfeld, T., Beverly, L., Bujak, A., Carey, D., Dukes, C., Duru, F., Feldman, G. J., Godley, A., Gülmez, E., Günaydın, Y. O., Gustafson, H. R., Gutay, L., Hartouni, E., Hanlet, P., Hansen, S., Heffner, M., Johnstone, C., Kaplan, D., Kamaev, O., Kilmer, J., Klay, J., Kostin, M., Lange, D., Ling, J., Longo, M. J., Lu, L. C., Materniak, C., Messier, M. D., Meyer, H., Miller, D. E., Mishra, S. R., Nelson, K., Nigmanov, T., Norman, A., Onel, Y., Paley, J. M., Park, H. K., Penzo, A., Peterson, R. J., Raja, R., Rajaram, D., Ratnikov, D., Rosenfeld, C., Rubin, H., Seun, S., Solomey, N., Soltz, R., Swallow, E., Schmitt, R., Subbarao, P., Torun, Y., Tope, T. E., Wilson, K., Wright, D., Wu, K.
Publikováno v:
Nucl.Instrum.Meth.A615:27-32,2010
The two most recent and precise measurements of the charged kaon mass use X-rays from kaonic atoms and report uncertainties of 14 ppm and 22 ppm yet differ from each other by 122 ppm. We describe the possibility of an independent mass measurement usi
Externí odkaz:
http://arxiv.org/abs/0909.0971
Autor:
Donati, JF, Howarth, ID, Jardine, MM, Petit, P, Catala, C, Landstreet, JD, Bouret, JC, Alecian, E, Barnes, JR, Forveille, T, Paletou, F, Manset, N
We report the discovery of a medium-strength (~0.5kG) magnetic field on the young, massive star tauSco (B0.2V), which becomes the third-hottest magnetic star known. Circularly polarized Zeeman signatures are clearly detected in observations collected
Externí odkaz:
http://arxiv.org/abs/astro-ph/0606156
Publikováno v:
Science 311 (2006) 633-635
Understanding how cool stars produce magnetic fields within their interiors is crucial for predicting the impact of such fields, such as the activity cycle of the Sun. In this respect, studying fully convective stars enables us to investigate the rol
Externí odkaz:
http://arxiv.org/abs/astro-ph/0602069
Autor:
Akerib, DS, Barnes Jr, PD, Bauer, DA, Brink, PL, Cabrera, B, Caldwell, DO, Clarke, RM, Da Silva, A, Davies, AK, Dougherty, BL, Irwin, KD, Gaitskell, RJ, Golwala, SR, Haller, EE, Jochum, J, Knowlton, WB, Kuzminov, V, Nam, SW, Novikov, V, Penn, MJ, Perera, TA, Ross, RR, Sadoulet, B, Schnee, RW, Shutt, T, Smith, A, Sonnenschein, AH, Spadafora, AL, Stockwell, WK, Yellin, S, Young, BA
Publikováno v:
Nucl.Phys.Proc.Suppl.70:64-68,1999
We are conducting an experiment to search for WIMPs, or weakly-interacting massive particles, in the galactic halo using terrestrial detectors. This generic class of hypothetical particles, whose properties are similar to those predicted by extension
Externí odkaz:
http://arxiv.org/abs/astro-ph/9712343
Autor:
Caleb C. Roth, Randolph D. Glickman, Stacey L. Martens, Ibtissam Echchgadda, Hope T. Beier, Ronald A. Barnes, Jr., Bennett L. Ibey
Publikováno v:
Biochemistry and Biophysics Reports, Vol 9, Iss C, Pp 302-309 (2017)
Background: Exposure of cells to very short (
Externí odkaz:
https://doaj.org/article/eff04149c7dd45189142633273613c30
Autor:
Seonsu Lee1, Barnes, Jr., James H.2
Publikováno v:
Journal of Advertising Research. Dec89/Jan90, Vol. 29 Issue 6, p25-30. 6p.