Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Tony S. Pan"'
Autor:
Tony S. Pan, Hsin-I Lu, Arvind Kannan, Rich Gorski, Yong Sun, Max N. Mankin, Andrew T. Koch, Clark Stephen E, Andrew R. Lingley, Morgan Monroe
Publikováno v:
2017 30th International Vacuum Nanoelectronics Conference (IVNC).
We used photolithography to fabricate nanoscale grids in proximity to a metal electrode. Such nanoscale grids can be used to mitigate the space charges in the inter-electrode region of a thermionic converter. The nanoscale dimensions together with lo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b7d83d83326f83170d83597b00d2855f
https://doi.org/10.1109/ivnc.2017.8051596
https://doi.org/10.1109/ivnc.2017.8051596
Autor:
Abraham Loeb, Tony S. Pan
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 435:L33-L37
Current surveys are underway to utilize gravitational lensing by galaxy clusters with Einstein radii >35" in the search for the highest redshift galaxies. Associated supernova from the epoch of reionization would have their fluxes boosted above the d
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6ef81ab7ef1c12bc8e846e07001a2786
https://doi.org/10.1093/mnrasl/slt089
https://doi.org/10.1093/mnrasl/slt089
Publikováno v:
2016 29th International Vacuum Nanoelectronics Conference (IVNC).
We developed a fabrication process that incorporates self-aligned double patterning to produce nanoscale electrostatic grids in close proximity to an electrode. These nanoscale grids can be used to mitigate the effects of space charge in the inter-el
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5ee658a21509992b0ef693ea88e77e38
https://doi.org/10.1109/ivnc.2016.7551465
https://doi.org/10.1109/ivnc.2016.7551465
Autor:
Max N. Mankin, Tony S. Pan
Publikováno v:
2016 IEEE International Vacuum Electronics Conference (IVEC).
We present the first nano- and microfabrication of vacuum microelectronic components incorporating lanthanum hexaboride (LaB 6 ), a refractory low work function material with high electron emissivity. We design novel fabrication processes which yield
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8078bc8fe72811d28218d0c1db111cb5
https://doi.org/10.1109/ivec.2016.7561801
https://doi.org/10.1109/ivec.2016.7561801
Autor:
Tony S. Pan, Abraham Loeb
Publikováno v:
Monthly Notices of the Royal Astronomical Society: Letters. 425:L91-L95
We examine the possibility that very massive stars greatly exceeding the commonly adopted stellar mass limit of 150 Msun may be present in young star clusters in the local universe. We identify ten candidate clusters, some of which may host stars wit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::82c08b6bbdf669fdb047e83ccc08f146
https://doi.org/10.1111/j.1745-3933.2012.01308.x
https://doi.org/10.1111/j.1745-3933.2012.01308.x
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 423:2203-2208
Stars with helium cores between ~64 and 133 M_sun are theoretically predicted to die as pair-instability supernovae. This requires very massive progenitors, which are theoretically prohibited for Pop II/I stars within the Galactic stellar mass limit
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::f230a816256af539f0679b309d3a570b
https://doi.org/10.1111/j.1365-2966.2012.21030.x
https://doi.org/10.1111/j.1365-2966.2012.21030.x
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 422:2701-2711
Pristine stars with masses between ~140 and 260 M_sun are theoretically predicted to die as pair-instability supernovae. These very massive progenitors could come from Pop III stars in the early universe. We model the light curves and spectra of pair
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5ed2d2b04022924036a62c7542c4fb7d
https://doi.org/10.1111/j.1365-2966.2012.20837.x
https://doi.org/10.1111/j.1365-2966.2012.20837.x
For supernova powered by the conversion of kinetic energy into radiation due to the interactions of the ejecta with a dense circumstellar shell, we show that there could be X-ray analogues of optically super-luminous SNe with comparable luminosities
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b79b6cda6aeec20b0e23c52c88ccd087
http://arxiv.org/abs/1303.6958
http://arxiv.org/abs/1303.6958
