Zobrazeno 1 - 10
of 2 937
pro vyhledávání: '"Bowen D"'
Autor:
Tyagi, S., Dreyer, M., Bowen, D., Hinkel, D., Taylor, P. J., Friedman, A. L., Butera, R. E., Krafft, C., Mayergoyz, I.
Spin-momentum locking in the surface mode of topological insulators (TI) leads to the surface accumulation of spin-polarized electrons caused by bias current flows through TI samples. Here, we demonstrate that scanning tunneling microscopy can be use
Externí odkaz:
http://arxiv.org/abs/2004.03563
Autor:
Tyagi, S., Dreyer, M., Bowen, D., Hinkel, D., Taylor, P. J., Friedman, A. L., Butera, R. E., Krafft, C., Mayergoyz, I.
The results of scanning tunneling microscopy experiments using iron-coated tungsten tips and current-carrying bismuth selenide ($Bi_2Se_3$) samples are reported. Asymmetry in tunneling currents with respect to the change in the direction of bias curr
Externí odkaz:
http://arxiv.org/abs/1911.00162
Autor:
Abou Kamar, S., Aga, Y. S., de Bakker, M., van den Berg, V. J., Strachinaru, M., Bowen, D., Frowijn, R., Akkerhuis, K. M., Brugts, J. J., Manintveld, O., Umans, V., Geleijnse, M., de Boer, R. A., Boersma, E., Kardys, I., van Dalen, B. M.
Publikováno v:
Clinical Research in Cardiology; Sep2024, Vol. 113 Issue 9, p1306-1316, 11p
Akademický článek
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Autor:
Bowen, D. V., Chelouche, D., Jenkins, E. B., Tripp, T. M., Pettini, M., York, D. G., Frye, B. L.
We present Hubble Space Telescope far-UV spectra of 4 QSOs whose sightlines pass through the halo of NGC 1097 at impact parameters of 48 -165 kpc. NGC 1097 is a nearby spiral galaxy that has undergone at least two minor merger events, but no apparent
Externí odkaz:
http://arxiv.org/abs/1605.04907
Autor:
Platzbecker, U., Fenaux, P. *, Adès, L., Giagounidis, A., Santini, V., van de Loosdrecht, A.A., Bowen, D., de Witte, T., Garcia-Manero, G., Hellström-Lindberg, E., Germing, U., Stauder, R., Malcovati, L., Sekeres, Mikkael A., Steensma, David P., Gloaguen, S.
Publikováno v:
In Blood 7 March 2019 133(10):1020-1030
Publikováno v:
In Applied Acoustics 1 January 2019 143:84-99
We present the results from our 21-cm absorption survey of a sample of 5 quasar-galaxy pairs (QGPs), with the redshift of the galaxies in the range 0.03
Externí odkaz:
http://arxiv.org/abs/1007.0288
We present a brief summary of results from our FUSE program designed to study OVI absorption in the disk of the Milky Way. As a full analysis of our data has now been published, we focus on the improvements that FUSE afforded us compared to Copernicu
Externí odkaz:
http://arxiv.org/abs/0902.1989