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@arXiv_astrophGA_bot@mastoxiv.page
2026-09-09 09:21:56

Detection prospects for heavy WIMP dark matter around M31* in microwave band
Andrei E. Egorov
arxiv.org/abs/2609.08771 arxiv.org/pdf/2609.08771 arxiv.org/html/2609.08771
arXiv:2609.08771v1 Announce Type: new
Abstract: This work analyzes the detection prospects for weakly interacting massive particles (WIMPs) in dark matter (DM) density spike around the supermassive black hole (SMBH) in Andromeda galaxy M31 in microwave band. WIMP annihilation produces relativistic electrons and positrons, which generate the synchrotron emission in strong magnetic field of the accretion flow medium at microwave frequencies. Properties of this emission, as well as their dependence on DM and medium parameters, were modeled. Atacama Large Millimeter Array (ALMA) sensitivity to this emission and underlying WIMP parameters was estimated. It was obtained that M31* in microwave band represents the unique target, where DM spike signal can be detected in case of realistic spike and halo density profiles. In such case ALMA may reach the thermal s-wave annihilating WIMPs with masses up to around 1 TeV with just 10--100 hours exposure. Optimistic parameter configurations may allow probing all possible WIMP masses up to 100 TeV. Related systematic uncertainties are discussed.
toXiv_bot_toot

@stargazersmith@social.linux.pizza
2026-08-04 13:14:36

space.com/astronomy/mars/signi

@macandi@social.heise.de
2026-09-04 11:08:07

PCIe 6.0 oder nicht: Verwirrung um Mac-Studio-Specs
Apple hatte in seiner Pressemitteilung zum neuen Mac Studio kurzzeitig erwähnt, dass die Maschinen mit PCIe 6.0 erscheinen. Das wurde inzwischen gestrichen.

@Dragofix@veganism.social
2026-09-02 23:48:22

Nepal floods highlight growing glacier risks in warming Himalayas news.mongabay.com/short-articl

@manawyrm@chaos.social
2026-08-03 09:19:56

Let's play a game:
Post the oldest image of your "battle station" / computer setup that you have.
Ideally, post some specs of the system if you can remember.
I'll start:
- photo from 2003
- Pentium II, 350MHz
- 3DFX Voodoo Banshee
- 1024x768 17" Eizo CRT
- Iomega Zip drive, 100MB via Parallel port (*click!*)
- SCSI Scanner hidden away in the background
I think the Mac was a Power Macintosh 6300, but I'm not 100…

2 computers, sitting on a carpeted floor, one PC tower with a ZIP drive on top, one Macintosh, 2 keyboards, 1 mouse, a 17" CRT screen
@arXiv_astrophGA_bot@mastoxiv.page
2026-09-09 11:30:55

Replaced article(s) found for astro-ph.GA. arxiv.org/list/astro-ph.GA/new
[3/4]:
- Characterising the Globular Cluster Systems of Three Local Group Dwarf Galaxies: NGC6822, NGC147 ...
McGill, Ferguson, Mackey, Crociati, Howell, Huxor, Irwin, McConnachie, Savino, Tanvir, Weisz
arxiv.org/abs/2608.28434 mastoxiv.page/@arXiv_astrophGA
- Magnetic Fields in Massive Star-forming Regions (MagMaR). IX. Radiative Torque Alignment and Disr...
Vineet Rawat, et al.
arxiv.org/abs/2609.03458 mastoxiv.page/@arXiv_astrophGA
- Rapid Growth of Intermediate-Mass Black Holes through Disk-induced Stellar Disruptions
Mengye Wang, Yiqiu Ma, Qingwen Wu, Boyuan Liu, Zijian Wang, Zhili Wang
arxiv.org/abs/2609.03701 mastoxiv.page/@arXiv_astrophGA
- Comparison of HMG and flat rotation velocities inferred from galaxy-galaxy weak lensing
Robert Monjo
arxiv.org/abs/2410.04258 mastoxiv.page/@arXiv_astrophCO
- Not-quite-primordial black holes
Wenzer Qin, Soubhik Kumar, Priyamvada Natarajan, Neal Weiner
arxiv.org/abs/2506.13858 mastoxiv.page/@arXiv_astrophCO
- Constraining fuzzy dark matter with the 21-cm power spectrum from Cosmic Dawn and Reionization
Shihang Liu, Yilin Liu, Bowen Peng, Mengzhou Xie, Zelong Liu, Bohua Li, Yi Mao
arxiv.org/abs/2508.10176 mastoxiv.page/@arXiv_astrophCO
- Using Strong Lensing to Detect Subhalos with Steep Inner Density Profiles
Kassidy E. Kollmann, James W. Nightingale, Mariangela Lisanti, Andrew Robertson, Oren Slone
arxiv.org/abs/2510.17956 mastoxiv.page/@arXiv_astrophCO
- Axion Constraints from White Dwarf Cooling in 47 Tucanae
Leesa Fleury, Alysa Obertas, Harvey Richer, Jeremy Heyl
arxiv.org/abs/2511.21676 mastoxiv.page/@arXiv_astrophSR
- Frequency shift and viewing direction variations in gravitational lensing
Miko{\l}aj Korzy\'nski, Mateusz Kulejewski
arxiv.org/abs/2601.13912 mastoxiv.page/@arXiv_astrophCO
- WIMP Dark Matter Searches in Reticulum II Using MeerKAT
Shibre Semane, Geoff Beck, Sphesihle Makhathini, Marco Regis, Gianni Bernardi
arxiv.org/abs/2603.06385 mastoxiv.page/@arXiv_astrophCO
toXiv_bot_toot

@cosmos4u@scicomm.xyz
2026-10-09 22:04:57

On the coronal origin of magnetic switchbacks in the #SolarWind: nature.com/articles/s41550-026 -> Solar Orbiter tracks origin of mysterious magnetic switchbacks: esa.int/Science_Exploration/Sp

@aardrian@toot.cafe
2026-09-23 14:57:53

[1/2]
Anyone used / heard of Aloud (“The first 508 audit that actually listens”)?
github.com/IRS-Public/aloud
It’s a CC0 project by the IRS that seems to want to be JAWS Inspect for native apps.
My look at README shows it’s got potential but may be grounded in misunderstandin…

@arXiv_astrophCO_bot@mastoxiv.page
2026-08-05 08:12:53

Modified Cosmological Expansion and the JWST CMB Optical Depth Tension in Self Interaction Gravity
Subhadeep Mukherjee, Shashank Shekhar Pandey, A. S. Majumdar
arxiv.org/abs/2608.03470 arxiv.org/pdf/2608.03470 arxiv.org/html/2608.03470
arXiv:2608.03470v1 Announce Type: new
Abstract: Recent James Webb Space Telescope (JWST) observations favor an earlier and more efficient reionization history, leading to Thomson-scattering optical depths larger than those inferred from the cosmic microwave background (CMB). We investigate whether this tension can be alleviated within the framework of self-interaction (SI) gravity by modifying the cosmological expansion history while retaining the standard astrophysical description of reionization. The SI gravity parameters are constrained through a Bayesian MCMC analysis of the Union3 Type Ia supernova and DESI DR2 Baryon Acoustic Oscillations (BAO) data. The resulting expansion history is then used to predict the ionization history and Thomson optical depth. We find that the predicted optical depth decreases from $\tau_{\rm{CMB}}\simeq0.076$ in $\Lambda$CDM to $\tau_{\rm{CMB}}\simeq0.061$, consistent with the Planck PR4 measurement within $1\sigma$, thereby substantially reducing the optical-depth tension.
toXiv_bot_toot

@peterhoneyman@a2mi.social
2026-08-01 03:20:24

i'm finna mail out some mix tapes this weekend so heads up michigan (ann arbor, ann arbor, and birmingham) and california (LA, oakland, SF).
hey, check out the splatter!

A stacked tower of six Norelco  cases, shot spine-on so you can read the labels:

"OW" — dark background, black lettering
"do listen" — dark background, white lettering
"Cal Tjader" — on a white FYDELITY-branded insert, magenta lettering
"sixties" — bold yellow lettering over a black/purple/red painted spine
"+ like" — black lettering over a cream spine splattered with blue and red paint, also FYDELITY-branded
"after work" — black lettering over a similar cream/blue/red splatter spine

The spla…
Six Norelco cases displayed face-out on mini easels against a brick wall:

Top left: cream/tan case with red splatter and blue drips (matches the "after work" splatter style)
Top center: black background with a scattering of colorful painted dots/circles — almost a night-sky or planetary look
Top right: white case with bold green, pink, and lavender curved bands, plus yellow at the edge
Bottom left: green background with a bold abstract design — black/blue swirl shapes outlined in red, with a r…