The HALO Collaboration today had its first collaboration meeting in many years. There was a lot to share and discuss!

We had great turnout of the collaboration for the hybrid meeting, with about 2/3 in the room and 1/3 online. It was exciting to discuss operations and analysis needs, new collaboration governance efforts, and to hear a new member institution proposal!

Here’s to being ready for the next galactic supernova!

#neutrinos #physics #collaboration #science

#Neutrinos from stars in the Milky Way: https://arxiv.org/abs/2510.07399 -> How Many Ghost Particles All the Milky Way’s Stars Send Towards Earth: https://news.ku.dk/all_news/2026/01/how-many-ghost-particles-all-the-milky-ways-stars-send-towards-earth/
Neutrinos from stars in the Milky Way

Neutrinos are produced during stellar evolution by means of thermal and thermonuclear processes. We model the cumulative neutrino flux expected at Earth from all stars in the Milky Way: the Galactic stellar neutrino flux (GS$ν$F). We account for the star formation history of our Galaxy and reconstruct the spatial distribution of Galactic stars by means of a random sampling procedure based on Gaia Data Release 2. We use the stellar evolution code $\texttt{MESA}$ to compute the neutrino emission for a suite of stellar models with solar metallicity and zero-age-main-sequence mass between $0.08M_\odot$ and $100\ M_\odot$, from their pre-main sequence phase to their final fates. We then reconstruct the evolution of the neutrino spectral energy distribution for each stellar model in our suite. The GS$ν$F lies between $\mathcal{O}(1)$ keV and $\mathcal{O}(10)$ MeV, with thermal (thermonuclear) processes responsible for shaping neutrino emission at energies smaller (larger) than $0.1$ MeV. Stars with mass larger than $\mathcal{O}(1\ M_\odot)$, located in the thin disk of the Galaxy, provide the largest contribution to the GS$ν$F. Moreover, most of the GS$ν$F originates from stars distant from Earth about $5-10$ kpc, implying that a large fraction of stellar neutrinos can reach us from the Galactic Center. Solar neutrinos and the diffuse supernova neutrino background have energies comparable to those of the GS$ν$F, challenging the detection of the latter. However, directional information of solar neutrino and GS$ν$F events, together with the annual modulation of the solar neutrino flux, could facilitate the GS$ν$F detection; this will kick off a new era for low-energy neutrino astronomy, also providing a novel probe to discover New Physics.

arXiv.org
In my dreams I fly

In my dreams I fly 25 September 2015 . The pied piper blew Into twists of my soul’s veins Tunes of the blessings . In mind no rat race Responded to dark musings Moving Time backwards . . Apprentice…

Geetha Balvannanathan's Blog - Isis Tratum

Aber was sind diese Neutrinos überhaupt? Ein kurzer Ausflug in die wunderbare Welt der Teilchenphysik schafft zumindest ein wenig mehr Klarheit.

#Physik #Neutrinos

https://t3n.de/news/schnellkurs-teilchenphysik-neutrinos-5-punkte-1673819/

Neutrinos für Einsteiger: Diese 5 Fakten machen dich zum Mini-Experten

Die Entdeckung hochenergetischer Neutrinos hat bei Forschenden für erhebliche Aufregung gesorgt. Warum eigentlich?

t3n Magazin

Aber was sind diese Neutrinos überhaupt? Ein kurzer Ausflug in die wunderbare Welt der Teilchenphysik schafft zumindest ein wenig mehr Klarheit.

#Physik #Neutrinos

https://t3n.de/news/teilchenphysik-5-fakten-neutrinos-1673819/

Neutrinos für Einsteiger: Diese 5 Fakten machen dich zum Mini-Experten

Die Entdeckung hochenergetischer Neutrinos hat bei Forschenden für erhebliche Aufregung gesorgt. Warum eigentlich?

t3n Magazin

The gluon cloud is exactly what QCD predicts.

“The HERA data are direct experimental proof that QCD describes nature,” Milner said.

But the young theory’s victory came with a bitter pill:

While QCD beautifully described the dance of short-lived quarks and gluons revealed by HERA’s extreme collisions,

the theory is useless for understanding the three long-lasting quarks seen in SLAC’s gentle bombardment.

QCD’s predictions are easy to understand only when the strong force is relatively weak.

And the strong force weakens only when quarks are extremely close together,
as they are in short-lived quark-antiquark pairs.

#Frank #Wilczek, #David #Gross and #David #Politzer identified this defining feature of QCD in 1973,
winning the Nobel Prize for it 31 years later.

But for gentler collisions like SLAC’s, where the proton acts like three quarks that mutually keep their distance,
these quarks pull on each other strongly enough that QCD calculations become impossible.

Thus, the task of further demystifying the three-quark view of the proton has fallen largely to experimentalists.
(Researchers who run “digital experiments,” in which QCD predictions are simulated on supercomputers,
have also made key contributions.)

And it’s in this low-resolution picture that physicists keep finding surprises.

Recently, a team led by #Juan #Rojo of the National Institute for Subatomic Physics in the Netherlands and VU University Amsterdam
analyzed more than 5,000 proton snapshots taken over the last 50 years,
using machine learning
to infer the motions of quarks and gluons inside the proton
in a way that sidesteps theoretical guesswork.

The new scrutiny picked up a background blur in the images that had escaped past researchers.

In relatively soft collisions just barely breaking the proton open,
most of the momentum was locked up in the usual three quarks:
two ups and a down.

But a small amount of momentum appeared to come from a “#charm#quark and charm #antiquark
— colossal elementary particles that each outweigh the entire proton by more than
one-third❗️

Short-lived charms frequently show up in the “quark sea” view of the proton
(gluons can split into any of six different quark types if they have enough energy).

But the results from Rojo and colleagues suggest that the charms have a more permanent presence,
making them detectable in gentler collisions.

In these collisions, the proton appears as a quantum mixture,
or superposition,
of multiple states:

An electron usually encounters the three lightweight quarks.

But it will occasionally encounter a rarer “molecule” of five quarks,
such as an up, down and charm quark grouped on one side and an up quark and charm antiquark on the other.

Such subtle details about the proton’s makeup could prove consequential.

At the Large Hadron Collider, physicists search for new elementary particles by bashing high-speed protons together and seeing what pops out;

to understand the results, researchers need to know what’s in a proton to begin with.

The occasional apparition of giant charm quarks would throw off the odds of making more exotic particles.

And when protons called #cosmic #rays hurtle here from outer space and slam into protons in Earth’s atmosphere,
charm quarks popping up at the right moments would shower Earth with extra-energetic #neutrinos, researchers calculated in 2021.

These could confound observers searching for high-energy neutrinos coming from across the cosmos.

Rojo’s collaboration plans to continue exploring the proton by searching for an imbalance between charm quarks and antiquarks.

And heavier constituents,
such as the #top quark, could make even rarer and harder-to-detect appearances.

Next-generation experiments will seek still more unknown features.

Physicists at Brookhaven National Laboratory hope to fire up the
"Electron-Ion Collider"
in the 2030s
and pick up where HERA left off,
taking higher-resolution snapshots that will enable the first 3D reconstructions of the proton.

The #EIC will also use spinning electrons to create detailed maps of the spins of the internal quarks and gluons,
just as SLAC and HERA mapped out their momentums.

This should help researchers to finally pin down the origin of the proton’s spin,
and to address other fundamental questions about the baffling particle that makes up most of our everyday world.

https://www.quantamagazine.org/inside-the-proton-the-most-complicated-thing-imaginable-20221019/

Inside the Proton, the ‘Most Complicated Thing’ Imaginable

The positively charged particle at the heart of the atom is an object of unspeakable complexity, one that changes its appearance depending on how it is probed. We’ve attempted to connect the proton’s many faces to form the most complete picture yet.

Quanta Magazine

La NASA ha lanzado con éxito su segundo globo científico desde la Antártida. La misión PUEO busca neutrinos de alta energía en el hielo para estudiar agujeros negros y fusiones de estrellas de neutrones.

#NASA #PUEO #Globo #Antártida #Neutrinos #Tutiempo

https://www.tutiempo.net/noticias/nasa-lanza-segundo-globo-desde-antartida-en-busca-de-neutrinos.html

La NASA lanza un segundo globo científico desde Antártida en busca de neutrinos

La NASA ha lanzado con éxito su segundo globo científico desde la Antártida. La misión PUEO busca neutrinos de alta energía en el hielo para estudiar agujeros negros y fusiones de estrellas de neutrones.

TuTiempo.net
No sterile neutrinos after all, say MicroBooNE physicists https://arstechni.ca/kfqK #sterileneutrinos #particlephysics #MicroBooNE #neutrinos #Science #Physics
No sterile neutrinos after all, say MicroBooNE physicists

There’s a less than 5 percent chance that earlier anomalies can be explained by fourth neutrino “flavor.”…

Ars Technica

Neutrino vindo do Sol transforma carbono em nitrogênio, numa espécie de alquimia cósmica.

O choque com os neutrinos fez átomos de carbono se transformarem em átomos de nitrogênio.

https://www.inovacaotecnologica.com.br/noticias/noticia.php?artigo=neutrino-transforma-carbono-nitrogenio

#ciencia #ciência #astronomia #espaço #universo #fisica #quimica #neutrinos #curiosidades

Neutrino vindo do Sol transforma carbono em nitrogênio

O choque com neutrinos vindos do Sol fez átomos de carbono se transformarem em átomos de nitrogênio, numa espécie de alquimia cósmica.

Site Inovação Tecnológica
Searches for Light #DarkMatter and Evidence of Coherent Elastic Neutrino-Nucleus Scattering of Solar #Neutrinos with the #LUX-ZEPLIN (LZ) Experiment: https://lz.lbl.gov/wp-content/uploads/sites/6/2025/12/LZ_Paper_Preprint_WS2025_v6.0_20251208.pdf / New Results from the LZ Dark Matter Experiment (recordings of 4 talks): https://vimeo.com/1136215171 -> LZ Sets a World’s Best in the Hunt for Galactic Dark Matter and Gets a New Look at Neutrinos from the Sun’s Core: https://newscenter.lbl.gov/2025/12/08/lz-sets-a-worlds-best-in-the-hunt-for-galactic-dark-matter/