Tabletop extreme ultraviolet time‐of‐flight spectrometry for trace analysis of high ionization energy samples

2019 ◽  
Vol 33 (14) ◽  
pp. 1196-1206 ◽  
Author(s):  
Yunieski Arbelo ◽  
Davide Bleiner
Keyword(s):  
Trace Analysis ◽  
Ionization Energy ◽  
Extreme Ultraviolet ◽  
Time Of Flight ◽  
High Ionization

Synthesis and characterization of solution processable, high electron affinity molecular dopants

2021 ◽  
Author(s):  
Jan Saska ◽  
Nikolay E. Shevchenko ◽  
Goktug Gonel ◽  
Zaira I. Bedolla-Valdez ◽  
Rachel M. Talbot ◽  
...  
Keyword(s):  
Electron Affinity ◽  
Ionization Energy ◽  
Synthesis And Characterization ◽  
High Electron ◽  
High Electron Affinity ◽  
High Ionization ◽  
Solution Processable

New organic-soluble dopants have record high electron affinity values and show outstanding doping performance with high ionization energy co-polymers.

scholarly journals EUV Radiation from B Stars: The Broad Implications for Stellar and Interstellar Astronomy

1996 ◽  
Vol 152 ◽  
pp. 367-374
Author(s):  
Joseph P. Cassinelli
Keyword(s):  
Variable Star ◽  
Extreme Ultraviolet ◽  
Early Type ◽  
Large Excess ◽  
Continuum Radiation ◽  
B Stars ◽  
Lyman Continuum ◽  
High Ionization ◽  
Early Type Stars ◽  
Warm Ionized Medium

Observations made with the Extreme Ultraviolet Explorer (EUVE) of the two bright stars ϵ CMa (B2 II) and β CMa (Bl II-III) are discussed. The photospheres show excess EUV radiation. The wind of ϵ CMa exhibits the Bowen Fluorescence mechanism, along with high ionization stages that help explain the nature of the wind shocks. The pulsation and beat phenomena exhibited by the variable star β CMa suggest that deposition of residual pulsation energy might heat and modify the structure of the atmospheres of early-type stars near the β Cephei strip. The possibility that many other B stars show a large excess Lyman continuum radiation is considered as a possible source of the ionization of the warm ionized medium (WIM) in the galactic ISM.

scholarly journals π± Spectra in Au+Au Collisions at $\sqrt{s_{\rm NN}}=62.4\ {\rm GeV}$

2005 ◽  
Vol 20 (16) ◽  
pp. 3783-3785 ◽  
Author(s):  
◽  
Zhangbu Xu
Keyword(s):  
Transverse Momentum ◽  
Energy Loss ◽  
Ionization Energy ◽  
Time Projection Chamber ◽  
Time Of Flight ◽  
Particle Identification ◽  
Resistive Plate Chamber ◽  
Ionization Energy Loss ◽  
Charged Pions ◽  
Time Projection

The combination of the ionization energy loss (dE/dx) from Time Projection Chamber (TPC) at ≃ 8% resolution and multi-gap resistive plate chamber time-of-flight (TOF) at 85ps provides powerful particle identification. We present spectra of identified charged pions from transverse momentum pT≃0.2 GeV/c to 7-8 GeV/c in Au + Au collisions at [Formula: see text]. Physics implications will be discussed.

scholarly journals Elongation of extreme ultraviolet (at 13.5 nm) emission with time-of-flight controlled discharges and lateral fuel injection

2008 ◽  
Vol 104 (5) ◽  
pp. 053306 ◽  
Author(s):  
Tomonao Hosokai ◽  
Takuma Yokoyama ◽  
Alexei Zhidkov ◽  
Hiroto Sato ◽  
Eiki Hotta ◽  
...  
Keyword(s):  
Fuel Injection ◽  
Extreme Ultraviolet ◽  
Time Of Flight
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