Zobrazeno 1 - 10
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pro vyhledávání: '"Taylor, James P"'
Autor:
Pandey, Atul, Rigvedi, Prajwal, Lesne, Edouard, Deka, Jitul, Yoon, Jiho, Hoppe, Wolfgang, Koerner, Chris, Pal, Banabir, Taylor, James M., Parkin, Stuart S. P., Woltersdorf, Georg
Antiferromagnets that display very small stray magnetic field are ideal for spintronic applications. Of particular interest are non-collinear, chiral antiferromagnets of the type Mn3X (X=Sn, Ge), which display a large magnetotransport response that i
Externí odkaz:
http://arxiv.org/abs/2409.15533
Autor:
Pandey, Atul, Deka, Jitul, Yoon, Jiho, Koerner, Chris, Dreyer, Rouven, Taylor, James M., Parkin, Stuart S. P., Woltersdorf, Georg
The anomalous Nernst effect (ANE) gives rise to an electrical response transverse to the magnetization and an applied temperature gradient in a magnetic metal. A nanoscale temperature gradient can be generated by the use of a laser beam applied to th
Externí odkaz:
http://arxiv.org/abs/2407.13028
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 532, Issue 2, August 2024, Pages 2521-2533
Galaxy cluster abundance measurements provide a classic test of cosmology. They are most sensitive to the evolved amplitude of fluctuations, usually expressed as $S_8 = \sigma_8\sqrt{\Omega_m/0.3}$. Thus, abundance constraints exhibit a strong degene
Externí odkaz:
http://arxiv.org/abs/2407.01661
Cosmological parameters such as $\Omega_{\rm{M}}$ and $\sigma_{8}$ can be measured indirectly using various methods, including galaxy cluster abundance and cosmic shear. These measurements constrain the composite parameter $S_{8}$, leading to degener
Externí odkaz:
http://arxiv.org/abs/2406.17849
Autor:
Haggar, Roan, De Luca, Federico, De Petris, Marco, Sazonova, Elizaveta, Taylor, James E., Knebe, Alexander, Gray, Meghan E., Pearce, Frazer R., Contreras-Santos, Ana, Cui, Weiguang, Kuchner, Ulrike, Paun, Robert A. Mostoghiu, Power, Chris
Numerous metrics exist to quantify the dynamical state of galaxy clusters, both observationally and within simulations. Many of these correlate strongly with one another, but it is not clear whether all of these measures probe the same intrinsic prop
Externí odkaz:
http://arxiv.org/abs/2406.15555
Autor:
Taylor, James
For a finite extension $F$ of $\mathbb{Q}_p$ and $n \geq 1$, let $D$ be the division algebra over $F$ of invariant $1/n$ and let $G^0$ be the subgroup of $\text{GL}_n(F)$ of elements with norm $1$ determinant. We show that the action of $D^\times$ on
Externí odkaz:
http://arxiv.org/abs/2406.14543
Autor:
Dashpute, Aniket, Wang, Jiazhang, Taylor, James, Cossairt, Oliver, Veeraraghavan, Ashok, Willomitzer, Florian
Event-based structured light systems have recently been introduced as an exciting alternative to conventional frame-based triangulation systems for the 3D measurements of diffuse surfaces. Important benefits include the fast capture speed and the hig
Externí odkaz:
http://arxiv.org/abs/2311.09652
Publikováno v:
Monthly Notices of the Royal Astronomical Society, Volume 527, Issue 2, January 2024, Pages 3459-3473
Dark matter haloes grow at a rate that depends on the value of the cosmological parameters $\sigma_8$ and $\Omega_{\rm m}$ through the initial power spectrum and the linear growth factor. While halo abundance is routinely used to constrain these para
Externí odkaz:
http://arxiv.org/abs/2311.03580
Dwarf galaxies are important tracers of small-scale cosmological structure, yet much of our knowledge about these systems comes from the limited sample of dwarf galaxies within the Local Group. To make a comprehensive inventory of dwarf populations i
Externí odkaz:
http://arxiv.org/abs/2310.17085
A growing body of evidence suggests that the central density of cuspy dark matter subhaloes is conserved in minor mergers. However, empirical models of subhalo evolution, calibrated from simulations, often assume a drop in the central density. Since
Externí odkaz:
http://arxiv.org/abs/2308.00830