Tootfinder

Octopus’ Kraken platform now manages 2 GW of demand flexibility, mostly from EV home chargers and EVs. If I understand correctly, more than half of these are EVs managed on the Octopus Intelligent Go tariff.
https://www.current-news.co.uk/ai-powered-…

AI-powered VPP Kraken reaches 2GW managed domestic assets
Octopus Energy’s Kraken now orchestrates over 2GW of domestic power from EVs, home batteries and heat pumps, the company has announced.

It amazes me that people still claim that Israel's actions are entirely about defense, or hostages.
“The fact that there are already 50,000 dead in Gaza is necessary and required for future generations. For everything that happened on October 7, for every person on October 7, 50 Palestinians need to die. It does not matter now if they are children. I am not speaking from revenge. I am speaking to future generations. They need a Nakba from time to time to feel the price. There is no…

Ok dan ...
Je stuurt op 1 oktober vorig jaar aan alle betrokkenen een brief dat je geen enkele verantwoordelijkheid meer kunt dragen voor de inmiddels ontstane situatie van de gezondheid. Wordt dat door vrijwel alle berokkenen voortdurend verder genegeerd. En krijg je aan het eind de rekening.
Oja ... En als je niet akkoord gaat dan ...

#Steady-CommunityContent
Seit Oktober 2024 haben #Mieter in Deutschland Anspruch auf die Zustimmung ihres #Vermieters zur Installation eines

Steckersolargeräte: Rechte und Förderung zu Balkonkraftwerken (1/n)
Du bist Mieter*in und willst Solarstrom? Erfahre, wie Du ein Balkonkraftwerk installierst – mit Tipps zu Genehmigung & Förderung.

A Data-constrained Magnetohydrodynamic Simulation of Successive X-class Flares in Solar Active Region 13842. II. Dynamics of the Solar Eruption Associated with the X9.0 Solar Flare
Keitarou Matsumoto, Satoshi Inoue, Keiji Hayashi, Nian Liu, Ying Wang, Jeongwoo Lee, Ju Jing, Haimin Wang
https://arxiv.org/abs/2508.07988

A Data-constrained Magnetohydrodynamic Simulation of Successive X-class Flares in Solar Active Region 13842. II. Dynamics of the Solar Eruption Associated with the X9.0 Solar Flare
Active region NOAA 13842 produced two successive solar flares: an X7.1-class flare on October 1, 2024, and an X9.0-class flare on October 3, 2024. This study continues our previous simulation work that successfully reproduced the X7.1-class solar flare (Matsumoto et al. 2025). In this study, we performed a data-constrained magnetohydrodynamic (MHD) simulation using the nonlinear force-free field (NLFFF) as the initial condition to investigate the X9.0-class solar flare. The NLFFF showed the she…

This https://arxiv.org/abs/2410.03612 has been replaced.
initial toot: https://mastoxiv.page/@arXiv_…

Resurrecting Gravitational Vector Modes and their Magnetogenesis
We revisit the presence of primordial gravitational vector modes (V-modes) and their sourcing of primordial magnetic fields (PMF), i.e. magnetogenesis. As the adiabatic vector mode generically decays with expansion, we consider exotic initial conditions which circumvent this issue and lead to observational imprints. The first initial condition is an isocurvature mode between photons and neutrinos vorticities, and the second one is a non-trivial initial condition on the neutrino octupole. Both t…

IceCat-2: Updated IceCube Event Catalog of Alert Tracks
Angela Zegarelli (for the IceCube Collaboration), Anna Franckowiak (for the IceCube Collaboration), Giacomo Sommani (for the IceCube Collaboration), Nora Valtonen-Mattila (for the IceCube Collaboration), Tianlu Yuan (for the IceCube Collaboration)
https://arxiv.org/abs/2507…

IceCat-2: Updated IceCube Event Catalog of Alert Tracks
We present preliminary results for IceCat-2, the second public catalog of IceCube Alert Tracks, which plans to build and improve upon the first release, IceCat-1. The initial catalog, last updated in October 2023, included all real-time alerts issued since 2016, as well as events observed by IceCube since the start of full-detector data collection in 2011 that would have triggered an alert if the program had been in place at that time. IceCat-2 plans to expand on this by incorporating all addit…

This https://arxiv.org/abs/2402.08161 has been replaced.
initial toot: https://mastoxiv.page/@ar…

The Monte Carlo Computational Summit -- October 25 & 26, 2023 -- Notre Dame, Indiana, USA
The Monte Carlo Computational Summit was held on the campus of the University of Notre Dame in South Bend, Indiana, USA on 25--26 October 2023. The goals of the summit were to discuss algorithmic and software alterations required for successfully porting respective code bases to exascale-class computing hardware, compare software engineering techniques used by various code teams, and consider the adoption of industry-standard benchmark problems to better facilitate code-to-code performance comp…

This https://arxiv.org/abs/2411.18943 has been replaced.
initial toot: https://mastoxiv.page/@arXiv_nuc…

Enhanced nuclear Schiff and electric dipole moments in nuclei with an octupole deformation
Deformed nuclei exhibit enhanced moments that violate time-reversal invariance ($T$) and parity ($P$). This paper focuses on the enhanced nuclear electric dipole moment (EDM) and Schiff moment present in nuclei with octupole deformation (pear-shaped nuclei). These moments, which are proportional to the octupole deformation, have a collective nature and are large in the intrinsic frame that rotates with the nucleus. However, in a state with definite angular momentum and parity, $T$ and $P$ conse…

This https://arxiv.org/abs/2503.20892 has been replaced.
initial toot: https://mastoxiv.page/@arXiv_…

X-ray polarization observations of NGC 2110 with IXPE
X-ray polarimetric observations from the Imaging X-ray Polarimeter Explorer (IXPE) is an excellent tool for probing the geometry and dynamics of X-ray emitting corona in active galactic nuclei (AGN). This work aims to investigate the geometry of the X-ray corona in the Seyfert 2 AGN, NGC 2110, using its first polarimetric observation with IXPE, conducted over a net exposure of 554 ks beginning on October 16, 2024. We performed a model-independent analysis of the 2-8 keV IXPE polarimetric observ…