4. Lower spin theory

Free Theory ◽  
2020 ◽  
pp. 224-265
Keyword(s):  
2021 ◽  
Vol 13 (1) ◽  
pp. 50-54
Author(s):  
Haya Alhummiany ◽  
Azzuliani Supangat

The present study describs the fabrication of hollow polyvinylidene fluoride-co-trifluoroethylene (P(VDF-TrFE)) nano-bundles by the template-assisted method. The P(VDF-TrFE) solution was spin-coated onto porous templates at four different rotation speeds, e.g., 1000 rpm, 2000 rpm, 3000 rpm, and 4000 rpm. The characteristics of the prepared nanostructures were evaluated to examine their morphological, structural, and hysteresis behaviors. All the P(VDF-TrFE) nanostructures were characterized as bundles rather than individual structures due to their agglomeration properties. The P(VDF-TrFE) nanostructures, which were synthesized at 4000 rpm, ensured a shorter length in comparison to the others fabricated at lower spin rates. Despite their different diameters and lengths, no clear difference was observed in the crystallinities of these nanostructures.


2011 ◽  
Vol 83 (3) ◽  
Author(s):  
Tokuei Sako ◽  
Josef Paldus ◽  
Atsushi Ichimura ◽  
Geerd H. F. Diercksen

2019 ◽  
Vol 99 (2) ◽  
Author(s):  
Tatsuo Azeyanagi ◽  
Stéphane Detournay ◽  
Max Riegler
Keyword(s):  

1981 ◽  
Vol 184 ◽  
pp. 333-350 ◽  
Author(s):  
S. Deser ◽  
P.K. Townsend ◽  
W. Siegel
Keyword(s):  

2021 ◽  
Vol 10 (1) ◽  
Author(s):  
Ryogo Kashiwagi ◽  
Shuhei Okamura ◽  
Shinya Iwanaga ◽  
Shunsuke Murakami ◽  
Koki Numata ◽  
...  

In tennis, the service is the only shot that a player can give himself without being influenced by his opponent, and it is said to be the most powerful and essential shot in the game to win the game (Kovacs and Ellenbecker, 2011). In this study, we will investigate the difference in speed and spin rate in services when a service is entered, when it is not entered, and when an ace is taken. Fourteen three-set singles matches of 20 participants in the ATP Challenger tournament were included in the analysis. The speed and spin rate was measured using the Trackman. The analysis included 1343 1st service balls. We compared the speed and spin rate for each IN, FAULT and ACE in the 1st service using one-way ANOVA. The speed of the 1st service, IN was significantly slower than that of FAULT and ACE. The spin rate of the 1st serve, IN had significantly more revolutions than the FAULT and ACE. The results of this study showed that the service was faster and lower spin rate when ACE was taken. However, it was found that the faster the speed of the service and the lower the spin rate, the higher the rate of FAULT. These considerations suggest that it is important to decide whether to take risks or play it safe, depending on the game situation at the time.


2021 ◽  
Vol 11 (5) ◽  
pp. 12761-12768

Titanium-doped zirconium oxide (mixed high-k) has been used as the gate oxide layer for the future generation metal oxide semiconductor devices. This mixed high-k layer was prepared by using Sol-Gel based spin-coated method. This mixed high-k layer’s chemical, structural, and initial electrical properties are investigated thoroughly. It is clearly confirmed that the suitable chemical composition and bond formation of the proposed mixed high-k layer from EDAX and FTIR analysis observations. The XRD spectra strengthened the presence of ZrTiO2. The measured dielectric constant of the proposed mixed high-k layer from the extracted C-V plots has been varying from 29.1 to 37.6 with respect to spin coating from 4000 to 6000 rpm. With lower spin rates, the leakage current is less.


2000 ◽  
Vol 15 (10) ◽  
pp. 1435-1451 ◽  
Author(s):  
M. KIRCHBACH

The Hilbert space ℋ3q of the three quarks with one excited quark is decomposed into Lorentz group representations. It is shown that the quantum numbers of the reported and "missing" resonances fall apart and populate distinct representations that differ by their parity or/and charge conjugation properties. In this way, reported and "missing" resonances become distinguishable. For example, resonances from the full listing reported by the Particle Data Group are accommodated by Rarita–Schwinger (RS) type representations [Formula: see text] with k=1, 3, and 5, the highest spin states being J=3/2-, 7/2+, and 11/2+, respectively. In contrast to this, most of the "missing" resonances fall into the opposite parity RS fields of highest-spins 5/2-, 5/2+, and 9/2+, respectively. Rarita–Schwinger fields with physical resonances as lower-spin components can be treated as a whole without imposing auxiliary conditions on them. Such fields do not suffer the Velo–Zwanziger problem but propagate causally in the presence of electromagnetic fields. The pathologies associated with RS fields arise basically because of the attempt to use them to describe isolated spin-J=k+½ states, rather than multispin-parity clusters. The positions of the observed RS clusters and their spacing are well explained trough the interplay between the rotational-like [Formula: see text]-rule and a Balmer-like [Formula: see text]-behavior.


1983 ◽  
Vol 212 (1) ◽  
pp. 173-188 ◽  
Author(s):  
V.O. Rivelles ◽  
J.G. Taylor
Keyword(s):  

2020 ◽  
Vol 500 (3) ◽  
pp. 2777-2785
Author(s):  
Beatriz Tucci ◽  
Antonio D Montero-Dorta ◽  
L Raul Abramo ◽  
Gabriela Sato-Polito ◽  
M Celeste Artale

ABSTRACT At z = 0, higher-spin haloes with masses above $\log (M_{\text{c}}/h^{-1}\, \text{M}_\odot)\simeq 11.5$ have a higher bias than lower-spin haloes of the same mass. However, this trend is known to invert below this characteristic crossover mass, Mc. In this paper, we measure the redshift evolution and scale dependence of halo spin bias at the low-mass end and demonstrate that the inversion of the signal is entirely produced by the effect of splashback haloes. These low-mass haloes tend to live in the vicinity of significantly more massive haloes, thus sharing their large-scale bias properties. We further show that the location of the redshift-dependent crossover mass scale Mc(z) is completely determined by the relative abundance of splashbacks in the low- and high-spin subpopulations. Once splashback haloes are removed from the sample, the intrinsic mass dependence of spin bias is recovered. Since splashbacks have been shown to account for some of the assembly bias signal at the low-mass end, our results unveil a specific link between two different secondary bias trends: spin bias and assembly bias.


2021 ◽  
Vol 922 (2) ◽  
pp. 270
Author(s):  
Brooks E. Kinch ◽  
Jeremy D. Schnittman ◽  
Scott C. Noble ◽  
Timothy R. Kallman ◽  
Julian H. Krolik

Abstract We present a survey of how the spectral features of black hole X-ray binary systems depend on spin, accretion rate, viewing angle, and Fe abundance when predicted on the basis of first-principles physical calculations. The power-law component hardens with increasing spin. The thermal component strengthens with increasing accretion rate. The Compton bump is enhanced by higher accretion rate and lower spin. The Fe Kα equivalent width grows sublinearly with Fe abundance. Strikingly, the Kα profile is more sensitive to accretion rate than to spin because its radial surface brightness profile is relatively flat, and higher accretion rate extends the production region to smaller radii. The overall radiative efficiency is at least 30%–100% greater than as predicted by the Novikov–Thorne model.


Sign in / Sign up

Export Citation Format

Share Document