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Adrian Thompson

@gooble-gabble.bsky.social

Theoretical Particle Physics Postdoc (Dark matter, neutrinos, and black holes) Prog metal enjoyer hymnoptera.bandcamp.com https://athompson-git.github.io/

699 Followers  |  302 Following  |  167 Posts  |  Joined: 07.11.2024  |  2.1858

Latest posts by gooble-gabble.bsky.social on Bluesky

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It’s a great moment to celebrate milestones at CFS — in more ways than one. Today we announced we’re done manufacturing one of our key magnets and putting it through a rigorous, month-long battery of performance tests — which it passed. 1/4

#PowerMoves

30.09.2025 13:34 — 👍 5    🔁 2    💬 1    📌 2

TIL if dealing with

(huge_number - huge_number2)

which can lead to machine precision noise in python computing, while mpmath can help a lot, sometimes just doing

(huge_number.astype('float64') - huge_number2.astype('float64'))

does the job more elegantly!

15.09.2025 22:49 — 👍 3    🔁 0    💬 0    📌 0
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Absolomb

listening to a banger open.spotify.com/track/49fTxU...

04.09.2025 15:32 — 👍 3    🔁 0    💬 0    📌 0
Graph Theory in State-Space
YouTube video by 2swap Graph Theory in State-Space

www.youtube.com/watch?v=YGLN...

31.08.2025 18:07 — 👍 1    🔁 0    💬 0    📌 0
Perhapsatron - Wikipedia

We've *gotta* revive this as a pet name for future colliders

en.wikipedia.org/wiki/Perhaps...

20.08.2025 03:45 — 👍 8    🔁 2    💬 0    📌 0

After >2 years, it's finally out!

30.07.2025 04:43 — 👍 2    🔁 0    💬 0    📌 0
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Coffee and paper review

21.07.2025 23:03 — 👍 3    🔁 0    💬 0    📌 0
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Toying around with some iNSPIRE API - trying to make a bubblemap of activity by subfield (counting papers with keyword in title by institution over the past 15 years)

17.07.2025 21:45 — 👍 0    🔁 0    💬 0    📌 0
Image of an optical module that was part of the
STRAW apparatus. The module is shown clean shortly
after deployment in 2018 (a.). An amount of buildup
is visible in the 2020 survey (b.). The final 2023 survey
shows a developed macro-fouling population, composed
primarily of hydroids (c.)

Image of an optical module that was part of the STRAW apparatus. The module is shown clean shortly after deployment in 2018 (a.). An amount of buildup is visible in the 2020 survey (b.). The final 2023 survey shows a developed macro-fouling population, composed primarily of hydroids (c.)

Cool ocean science work on "biofouling" for the Pacific One Neutrino Experiment :) 🧪⚛️

arxiv.org/abs/2507.09086

15.07.2025 16:17 — 👍 1    🔁 0    💬 0    📌 0
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Just got back from a visit underground at SURF, where we also heard a little about SABRE. Reminds me of this t-shirt:

14.07.2025 23:07 — 👍 2    🔁 0    💬 1    📌 0

Right there with ya Tao 😭
Though as Patrick put it, correlation != causation here, so the numbers shouldn't really change what we do or make us pessimistic - I think we keep writing good papers, talk to people, and apply anyways!

14.07.2025 20:46 — 👍 1    🔁 0    💬 0    📌 0

Absolutely, this is a mix of lots of career stages though I was more interested in cut-offs than the high h-index tail. And I think there is a bit of conditional probability here; I might feel less inclined to even apply if I have a low h-index / first postdoc

13.07.2025 22:23 — 👍 1    🔁 0    💬 0    📌 0
A histogram of number of faculty shortlists and faculty offers binned by citation count for papers with 10 authors or less, for 2024-2025 data.

A histogram of number of faculty shortlists and faculty offers binned by citation count for papers with 10 authors or less, for 2024-2025 data.

A similar effect shows up in citation counts > 500. I've heard that committes don't necessarily impose hard cut-offs, but numbers obviously help to make your case. Perhaps the more optimistic thing I can draw from all this is that you don't need to hit these numbers to get shortlisted.

13.07.2025 21:42 — 👍 1    🔁 0    💬 1    📌 0
A histogram of number of faculty shortlists and faculty offers binned by paper count for papers with 10 authors or less, for 2024-2025 data.

A histogram of number of faculty shortlists and faculty offers binned by paper count for papers with 10 authors or less, for 2024-2025 data.

Less so is the bias for high paper counts, although no offers were made to candidates with N(papers) < 17

13.07.2025 21:42 — 👍 0    🔁 0    💬 1    📌 0
A histogram of number of faculty shortlists and faculty offers binned by author h-index for papers with 10 authors or less, for 2024-2025 data.

A histogram of number of faculty shortlists and faculty offers binned by author h-index for papers with 10 authors or less, for 2024-2025 data.

Do metrics matter?

Some interesting statistics on faculty hires in hep-ph/th in the past two years, sourced from the rumor mill and inSPIRE data. For instance, there is a clear bias in offers to higher h-index ~ 15

13.07.2025 21:42 — 👍 3    🔁 0    💬 2    📌 0

Thanks for saying this part out loud, it's nice to know these practices are appreciated by others!

06.06.2025 18:26 — 👍 1    🔁 0    💬 0    📌 0
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[W190] Adrian Thompson: The Terrestrial Neutrino Lighthouse YouTube video by lawphysics

I will give a talk on #neutrinos from a #muoncollider and electroweak precision on Lawphysics this morning:
www.youtube.com/live/_fd6w7o...
🧪⚛️

04.06.2025 13:13 — 👍 2    🔁 0    💬 1    📌 0
Diagram of the Earth’s core, with an example dark
matter density profile superimposed. The solid-liquid boundary at 1200 km is the boundary between the inner core and
outer core, while a radius of 400 km is where the seismic data
we use loses sensitivity to the core’s structure (see text for details). Dashed arrows denote heat flow away from the center
of the Earth.

Diagram of the Earth’s core, with an example dark matter density profile superimposed. The solid-liquid boundary at 1200 km is the boundary between the inner core and outer core, while a radius of 400 km is where the seismic data we use loses sensitivity to the core’s structure (see text for details). Dashed arrows denote heat flow away from the center of the Earth.

Fun paper I noticed last night by Chris Cappiello and Tansu Daylan :D

Can a Dark Inferno Melt Earth's Core?
arxiv.org/abs/2505.24070

03.06.2025 00:12 — 👍 1    🔁 0    💬 0    📌 0
The Quantum Foundation Collection

Nice collection of historical landmarks in Quantum theory from APS: promo.aps.org/quantum-foun...

06.05.2025 21:42 — 👍 4    🔁 1    💬 0    📌 0
Goofy is the New Normal

Goofy is the New Normal

While I'm happy to have a paper out tonight myself, I can't *not* read this one, excited to learn that the author is likely a skateboarder:

arxiv.org/pdf/2505.00099

02.05.2025 01:57 — 👍 3    🔁 0    💬 0    📌 0
Duolingo screenshot showing the sentence "Neha's big toes are small"

Duolingo screenshot showing the sentence "Neha's big toes are small"

I just learned that our "big toes" in Hindi are expressed as the "foot's thumbs" (पैर का अंगूठा), amazing 😂

29.03.2025 03:04 — 👍 0    🔁 0    💬 0    📌 0
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LHCb paper on the first observation of CP violation in baryon decays, looks awesome!

arxiv.org/abs/2503.16954

24.03.2025 15:05 — 👍 3    🔁 1    💬 0    📌 0
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First constraints on QCD axion dark matter using James Webb Space Telescope observations I present the first constraints on QCD axion dark matter using measurements from the James Webb Space Telescope. By utilizing publicly available MIRI and NIRSpec blank-sky observations, originally col...

Nice! JWST, axions and the 0.1-1 eV window from Pinetti 🧪⚛️

arxiv.org/abs/2503.11753

19.03.2025 00:55 — 👍 10    🔁 2    💬 0    📌 0

Have fun and come back with merch!

16.03.2025 05:57 — 👍 1    🔁 0    💬 0    📌 0

Wow, bold!

07.03.2025 01:35 — 👍 0    🔁 0    💬 0    📌 0
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Misconceptions in Neutrino Oscillations in presence of a non-Unitary Mixing Deviations from unitarity of the CKM matrix in the quark sector are considered excellent windows to probe physics beyond the Standard Model. In its leptonic counterpart, the PMNS matrix, these searche...

Looks like a good paper to go through for my own education

arxiv.org/abs/2502.19480

03.03.2025 15:36 — 👍 1    🔁 0    💬 0    📌 0
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a man in a suit and tie with the words stop it above him ALT: a man in a suit and tie with the words stop it above him
19.02.2025 17:45 — 👍 30    🔁 0    💬 0    📌 0

I see - but here the authors study a hypothetical feebly interacting particle that would not get absorbed by the blanket, so in principle you could have a well-shielded detector trying to pick up a signal

19.02.2025 17:42 — 👍 2    🔁 0    💬 0    📌 0

Yeah, pretty crazy! Looks like it's all coming the high neutron flux, but I think they key is that they assumed 1 year of data taking = 1 year reactor on...that would take a high duty factor, not just test operations. I'm still reading tho...

19.02.2025 05:18 — 👍 0    🔁 0    💬 1    📌 0

I don't know enough about fusion reactors to know if what they assumed was gratuitous, but it looks like most of the sensitivities have a hard time competing with K->Pi+inv. constraints, right?

19.02.2025 04:19 — 👍 1    🔁 0    💬 1    📌 0

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