First Measurement of π+\pi^+-Ar and pp-Ar Total Inelastic Cross Sections in the Sub-GeV Energy Regime with ProtoDUNE-SP Data

Using data from the ProtoDUNE-SP detector at CERN, this paper reports the first measurements of the total inelastic cross sections for π+\pi^+-Ar and pp-Ar interactions in the sub-GeV energy regime, providing essential constraints for neutrino-argon interaction models critical to the upcoming DUNE experiment.

Original authors: DUNE Collaboration, S. Abbaslu, F. Abd Alrahman, A. Abed Abud, R. Acciarri, L. P. Accorsi, M. A. Acero, M. R. Adames, G. Adamov, M. Adamowski, C. Adriano, F. Akbar, F. Alemanno, N. S. Alex, L. Aliaga
Published 2026-05-28
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Original authors: DUNE Collaboration, S. Abbaslu, F. Abd Alrahman, A. Abed Abud, R. Acciarri, L. P. Accorsi, M. A. Acero, M. R. Adames, G. Adamov, M. Adamowski, C. Adriano, F. Akbar, F. Alemanno, N. S. Alex, L. Aliaga Soplin, K. Allison, M. Alrashed, A. Alton, R. Alvarez, T. Alves, A. Aman, H. Amar, P. Amedo, J. Anderson, D. A. Andrade, C. Andreopoulos, M. Andreotti, M. P. Andrews, F. Andrianala, S. Andringa, F. Anjarazafy, S. Ansarifard, D. Antic, M. Antoniassi, A. Aranda-Fernandez, T. Araya-Santander, L. Arellano, E. Arrieta Diaz, M. A. Arroyave, M. Artero Pons, J. Asaadi, M. Ascencio, A. Ashkenazi, D. Asner, L. Asquith, E. Atkin, D. Auguste, A. Aurisano, V. Aushev, D. Autiero, D. Ávila Gómez, M. B. Azam, F. Azfar, J. J. Back, Y. Bae, I. Bagaturia, L. Bagby, D. Baigarashev, S. Balasubramanian, A. Balboni, P. Baldi, W. Baldini, J. Baldonedo, B. Baller, B. Bambah, F. Barao, D. Barbu, G. Barenboim, P. Barham Alzás, G. J. Barker, W. Barkhouse, G. Barr, A. Barros, N. Barros, D. Barrow, J. L. Barrow, A. Basharina-Freshville, A. Bashyal, V. Basque, M. Bassani, D. Basu, C. Batchelor, L. Bathe-Peters, J. B. R. Battat, F. Battisti, J. Bautista, F. Bay, J. L. L. Bazo Alba, J. F. Beacom, E. Bechetoille, B. Behera, E. Belchior, B. Bell, G. Bell, L. Bellantoni, G. Bellettini, V. Bellini, O. Beltramello, A. Belyaev, C. Benitez Montiel, D. Benjamin, F. Bento Neves, J. Berger, S. Berkman, J. Bermudez, J. Bernal, P. Bernardini, A. Bersani, E. Bertholet, E. Bertolini, S. Bertolucci, M. Betancourt, A. Betancur Rodríguez, Y. Bezawada, A. T. Bezerra, A. Bhat, V. Bhatnagar, M. Bhattacharjee, S. Bhattacharjee, M. Bhattacharya, S. Bhuller, B. Bhuyan, S. Biagi, J. Bian, K. Biery, B. Bilki, M. Bishai, P. Bishop, A. Blake, F. D. Blaszczyk, G. C. Blazey, E. Blucher, A. Bodek, B. Bogart, J. Boissevain, S. Bolognesi, T. Bolton, L. Bomben, M. Bonesini, C. Bonilla-Diaz, A. Booth, F. Boran, C. Borden, R. Borges Merlo, N. Bostan, G. Botogoske, B. Bottino, R. Bouet, J. Boza, J. 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Original paper licensed under CC BY 4.0 (http://creativecommons.org/licenses/by/4.0/). This is an AI-generated explanation of the paper below. It is not written or endorsed by the authors. For technical accuracy, refer to the original paper. Read full disclaimer

Imagine you are trying to understand how a specific type of car (a neutrino) behaves when it crashes into a very specific, heavy wall made of liquid argon. To predict exactly how the car will crumple and what pieces will fly off, you need to know exactly how the wall reacts to different types of debris hitting it.

This paper is like a team of mechanics running a crash test to figure out exactly how argon (the wall) reacts when hit by two common types of debris: pions and protons (the debris).

Here is the breakdown of what they did and why it matters, using simple analogies:

1. The Big Goal: The "Crystal Ball" Problem

The scientists are building a giant experiment called DUNE (Deep Underground Neutrino Experiment). It's like a massive, high-tech camera buried deep underground, filled with 70,000 tons of liquid argon. Its job is to take pictures of neutrinos (ghostly particles) passing through.

However, when a neutrino hits an argon atom, it doesn't just stop; it creates a shower of other particles (like pions and protons). These new particles bounce around inside the argon nucleus before they escape. This is called a "Final State Interaction."

The Problem: The scientists didn't have a perfect "rulebook" for how these particles bounce around inside argon. They had to guess based on how they bounce off other materials (like carbon or lead). It's like trying to predict how a billiard ball will bounce off a pool table made of ice, but you've only ever studied how it bounces off wood. Your prediction might be wrong, and that mistake could ruin your measurement of the neutrino itself.

2. The Solution: The "Sandwich" Test

To fix this, they used a prototype detector called ProtoDUNE-SP. Think of this as a full-scale "mock-up" of the real camera, filled with liquid argon.

They didn't just wait for neutrinos to hit it. Instead, they fired a controlled beam of pions and protons directly into the liquid argon.

  • The Beam: Imagine a machine gun shooting tiny particles at the liquid argon.
  • The Trick: Usually, to measure how often a particle hits a target, you use a very thin sheet of material. But liquid argon is thick. If a particle hits the front, it might hit again before it exits.
  • The "Slicing" Method: To solve this, the scientists treated the liquid argon like a loaf of bread. They virtually sliced the path of the particle into thin "slices" of energy. They tracked the particle as it entered a slice, lost a little energy (like a car slowing down on a rough road), and either bounced out or crashed inside that specific slice. This allowed them to count exactly how many "crashes" happened at every specific speed.

3. The Results: Filling the "Missing Page"

The paper reports the first-ever measurements of how often pions and protons crash into argon atoms at specific speeds (energies) that are very common in neutrino experiments.

  • The Pion Test: They measured pions moving at speeds between 500 and 900 MeV (a specific unit of energy).
  • The Proton Test: They measured protons moving at speeds below 450 MeV.

The Analogy: Before this, the scientists were trying to bake a cake using a recipe that said "add some flour," but they didn't know how much. They had to guess based on recipes for other cakes. This paper finally gives them the exact measurement: "You need exactly 200 grams of argon-flour for this speed of particle."

4. What They Found

When they compared their new measurements to the computer simulations (the "rulebooks" they were using before), they found:

  • The simulations were actually pretty good! The new data matched the predictions from the Geant4 software (a standard physics simulation tool) very well.
  • However, having the real data is crucial. It's the difference between a chef guessing the taste of a dish and actually tasting it. Now, they have the "taste test" results for argon.

5. Why This Matters for the Future

The paper states that these measurements are essential for the DUNE experiment.

  • By knowing exactly how particles interact with argon, scientists can build better "rulebooks" (models).
  • Better rulebooks mean less guessing when they analyze neutrino data.
  • Less guessing means they can measure the properties of neutrinos (like their mass and how they change types) with much higher precision.

In Summary:
This paper is a "quality control" report. The scientists built a giant liquid argon tank, shot particles at it, and counted the collisions. They proved that their current computer models are mostly correct, but more importantly, they provided the first hard data to back those models up. This ensures that when the real DUNE experiment starts taking pictures of neutrinos, the scientists won't be misinterpreting the blurry parts of the image caused by the argon wall.

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