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First Measurement of Muon Neutrino Interactions at LHC

Scientists measure muon neutrino interactions for the first time at LHC.

FASER Collaboration, Roshan Mammen Abraham, Xiaocong Ai, John Anders, Claire Antel, Akitaka Ariga, Tomoko Ariga, Jeremy Atkinson, Florian U. Bernlochner, Tobias Boeckh, Jamie Boyd, Lydia Brenner, Angela Burger, Franck Cadoux, Roberto Cardella, David W. Casper, Charlotte Cavanagh, Xin Chen, Dhruv Chouhan, Andrea Coccaro, Stephane Débieux, Monica D'Onofrio, Ansh Desai, Sergey Dmitrievsky, Radu Dobre, Sinead Eley, Yannick Favre, Deion Fellers, Jonathan L. Feng, Carlo Alberto Fenoglio, Didier Ferrere, Max Fieg, Wissal Filali, Elena Firu, Ali Garabaglu, Stephen Gibson, Sergio Gonzalez-Sevilla, Yuri Gornushkin, Carl Gwilliam, Daiki Hayakawa, Michael Holzbock, Shih-Chieh Hsu, Zhen Hu, Giuseppe Iacobucci, Tomohiro Inada, Luca Iodice, Sune Jakobsen, Hans Joos, Enrique Kajomovitz, Hiroaki Kawahara, Alex Keyken, Felix Kling, Daniela Köck, Pantelis Kontaxakis, Umut Kose, Rafaella Kotitsa, Susanne Kuehn, Thanushan Kugathasan, Lorne Levinson, Ke Li, Jinfeng Liu, Yi Liu, Margaret S. Lutz, Jack MacDonald, Chiara Magliocca, Toni Mäkelä, Lawson McCoy, Josh McFayden, Andrea Pizarro Medina, Matteo Milanesio, Théo Moretti, Mitsuhiro Nakamura, Toshiyuki Nakano, Laurie Nevay, Ken Ohashi, Hidetoshi Otono, Hao Pang, Lorenzo Paolozzi, Pawan Pawan, Brian Petersen, Titi Preda, Markus Prim, Michaela Queitsch-Maitland, Hiroki Rokujo, André Rubbia, Jorge Sabater-Iglesias, Osamu Sato, Paola Scampoli, Kristof Schmieden, Matthias Schott, Anna Sfyrla, Davide Sgalaberna, Mansoora Shamim, Savannah Shively, Yosuke Takubo, Noshin Tarannum, Ondrej Theiner, Eric Torrence, Oscar Ivan Valdes Martinez, Svetlana Vasina, Benedikt Vormwald, Di Wang, Yuxiao Wang, Eli Welch, Monika Wielers, Yue Xu, Samuel Zahorec, Stefano Zambito, Shunliang Zhang

― 6 min read


Muon Neutrino Interaction Muon Neutrino Interaction Breakthrough reveal secrets of neutrinos. First-ever measurements achieved at LHC
Table of Contents

In a groundbreaking achievement, scientists have made the first measurement of muon neutrino interactions at the Large Hadron Collider (LHC). This remarkable feat involves studying how neutrinos interact with matter, specifically Tungsten, as they fly through our world largely unnoticed. These elusive particles are like that one friend who always shows up late to the party but still manages to have a remarkable impact.

What Are Muon Neutrinos?

Muon neutrinos are one type of neutrino, which are tiny particles that play a significant role in the universe. They are created when particles like pions and kaons decay. Neutrinos are incredibly light and interact very weakly with other matter, making them hard to detect. Imagine trying to catch a shadow: it's nearly impossible because they pass right through most things without leaving a trace.

The Goal of the Experiment

The primary objective of this experiment was to measure how often muon neutrinos interact with other particles in a material called tungsten. Scientists have been trying to understand the properties of neutrinos for many years, and this study aims to provide important data that could help clarify their behavior.

By focusing on the interactions of neutrinos, researchers can gain insights into the fundamental forces that govern the universe. The findings could have broad implications for several fields, including particle physics and even astrophysics.

The LHC: A Particle Physics Giant

The LHC is a massive particle accelerator located near Geneva, Switzerland. It is the largest and most powerful collider in the world, where protons crash into each other at incredible speeds. When these collisions occur, a variety of particles, including neutrinos, are produced. The LHC is like a cosmic mixing pot, stirring together components of the universe to uncover the secrets of nature.

The FASER Detector

To capture the interactions of muon neutrinos, scientists used a specialized detector known as FASER (ForwArd Search ExpeRiment). This detector is positioned in a tunnel about 480 meters from one of the collision points of the LHC. It's like placing a magnifying glass on the scene of a cosmic event, allowing researchers to zoom in on the tiny details of neutrino interactions.

FASER was designed to detect neutrinos without interference from other particles. It has an impressive setup, including layers of tungsten and electronic components that help identify neutrino events. Think of it as a very sophisticated fishing net designed to catch a specific type of fish (in this case, neutrinos) while letting everything else swim by unharmed.

The Experiment: How It Worked

During the experiment, scientists analyzed data collected from proton-proton collisions at the LHC. They focused on interactions within the detector that produced charged current muon neutrinos. By carefully filtering out other noise and background signals, they were able to identify a total of around 338 charged current muon neutrino interactions. It’s not unlike spotting a specific grain of sand on a beach.

The researchers had to ensure that they were indeed measuring muon neutrinos and not other particles, which is no small feat given that neutrinos are notoriously difficult to pin down. They used various techniques to distinguish the signals and reduce background noise from other sources.

Converting Data into Results

The data collected were analyzed in detail. Scientists needed to convert the observed interactions into a usable format. This involved "unfolding" the data, which is a fancy term for refining the observations to better understand underlying patterns. They created six bins based on neutrino energy to make sense of the results.

Through careful calculations, the researchers could then derive the interaction cross-section—a measure of how likely neutrinos are to interact with matter—as well as the differential neutrino flux, which describes how many neutrinos are coming from different energy levels.

The Results

The results showed that the observed muon neutrino interactions aligned well with predictions from the Standard Model of particle physics. This model acts like a map for physicists, guiding them through the complexities of the particle world.

The measurement covered a range of energies from low to high, marking a significant step forward in the field. The researchers could even estimate the contributions of neutrinos originating from pions and kaons, providing a clearer picture of where these particles come from and how they behave.

Implications of the Findings

These measurements have the potential to unlock new doors in understanding not just neutrinos but the universe as a whole. By studying how neutrinos interact, scientists could gain clues about phenomena we have yet to comprehend fully, including those weird cosmic occurrences that seem to defy explanation.

Additionally, this research bridges the gap between data from fixed-target experiments and astroparticle physics. It's a bit like connecting the dots in a complex puzzle, where each piece adds to a larger picture of how the universe operates.

Acknowledging the Team Effort

This groundbreaking work is the result of collaboration among many scientists and institutions around the world. The success of such experiments relies heavily on teamwork. While the LHC provides the cosmic playground, the people behind the scenes diligently work to ensure that every detail is captured and analyzed effectively.

The collaboration emphasizes the importance of sharing knowledge and resources in the scientific community. Just like in any successful venture, teamwork is crucial. It’s a reminder that behind every great discovery, there are countless hours of hard work and dedication from individuals committed to understanding the mysteries of the universe.

What Happens Next?

With the first measurement of muon neutrino interactions achieved, the scientific community is excited about what lies ahead. This research could pave the way for future experiments and studies that delve deeper into the nature of neutrinos and their role in the cosmos.

Scientists are likely to continue refining their techniques and expanding their understanding of neutrinos. As they gather more data and improve their methods, we can expect even more fascinating findings in the years to come.

A Bright Future for Neutrino Physics

As technology continues to advance, so too will our ability to study particles like neutrinos. The ongoing exploration of the smallest components of our universe promises to shed light on the fundamental questions that have puzzled humanity for centuries.

In the end, studying neutrinos is not just about understanding one particle; it's about grasping the very fabric of reality. Whether you're a scientist in a lab coat or just someone with a curious mind, the journey into the world of neutrinos is bound to be full of wonder and awe.

Conclusion

This first measurement of muon neutrino interactions at the LHC provides a gateway to a deeper understanding of the universe. With data revealing new insights into how these particles behave, scientists are one step closer to answering some of the most pressing questions in physics. And remember, the next time you feel small or insignificant, just think about the muon neutrinos that travel through you every day without you even knowing it. In the grand scheme of things, we're all a part of this vast cosmic dance, and now we have a little more insight into the rhythm.

Original Source

Title: First Measurement of the Muon Neutrino Interaction Cross Section and Flux as a Function of Energy at the LHC with FASER

Abstract: This letter presents the measurement of the energy-dependent neutrino-nucleon cross section in tungsten and the differential flux of muon neutrinos and anti-neutrinos. The analysis is performed using proton-proton collision data at a center-of-mass energy of $13.6 \, {\rm TeV}$ and corresponding to an integrated luminosity of $(65.6 \pm 1.4) \, \mathrm{fb^{-1}}$. Using the active electronic components of the FASER detector, $338.1 \pm 21.0$ charged current muon neutrino interaction events are identified, with backgrounds from other processes subtracted. We unfold the neutrino events into a fiducial volume corresponding to the sensitive regions of the FASER detector and interpret the results in two ways: We use the expected neutrino flux to measure the cross section, and we use the predicted cross section to measure the neutrino flux. Both results are presented in six bins of neutrino energy, achieving the first differential measurement in the TeV range. The observed distributions align with Standard Model predictions. Using this differential data, we extract the contributions of neutrinos from pion and kaon decays.

Authors: FASER Collaboration, Roshan Mammen Abraham, Xiaocong Ai, John Anders, Claire Antel, Akitaka Ariga, Tomoko Ariga, Jeremy Atkinson, Florian U. Bernlochner, Tobias Boeckh, Jamie Boyd, Lydia Brenner, Angela Burger, Franck Cadoux, Roberto Cardella, David W. Casper, Charlotte Cavanagh, Xin Chen, Dhruv Chouhan, Andrea Coccaro, Stephane Débieux, Monica D'Onofrio, Ansh Desai, Sergey Dmitrievsky, Radu Dobre, Sinead Eley, Yannick Favre, Deion Fellers, Jonathan L. Feng, Carlo Alberto Fenoglio, Didier Ferrere, Max Fieg, Wissal Filali, Elena Firu, Ali Garabaglu, Stephen Gibson, Sergio Gonzalez-Sevilla, Yuri Gornushkin, Carl Gwilliam, Daiki Hayakawa, Michael Holzbock, Shih-Chieh Hsu, Zhen Hu, Giuseppe Iacobucci, Tomohiro Inada, Luca Iodice, Sune Jakobsen, Hans Joos, Enrique Kajomovitz, Hiroaki Kawahara, Alex Keyken, Felix Kling, Daniela Köck, Pantelis Kontaxakis, Umut Kose, Rafaella Kotitsa, Susanne Kuehn, Thanushan Kugathasan, Lorne Levinson, Ke Li, Jinfeng Liu, Yi Liu, Margaret S. Lutz, Jack MacDonald, Chiara Magliocca, Toni Mäkelä, Lawson McCoy, Josh McFayden, Andrea Pizarro Medina, Matteo Milanesio, Théo Moretti, Mitsuhiro Nakamura, Toshiyuki Nakano, Laurie Nevay, Ken Ohashi, Hidetoshi Otono, Hao Pang, Lorenzo Paolozzi, Pawan Pawan, Brian Petersen, Titi Preda, Markus Prim, Michaela Queitsch-Maitland, Hiroki Rokujo, André Rubbia, Jorge Sabater-Iglesias, Osamu Sato, Paola Scampoli, Kristof Schmieden, Matthias Schott, Anna Sfyrla, Davide Sgalaberna, Mansoora Shamim, Savannah Shively, Yosuke Takubo, Noshin Tarannum, Ondrej Theiner, Eric Torrence, Oscar Ivan Valdes Martinez, Svetlana Vasina, Benedikt Vormwald, Di Wang, Yuxiao Wang, Eli Welch, Monika Wielers, Yue Xu, Samuel Zahorec, Stefano Zambito, Shunliang Zhang

Last Update: 2024-12-04 00:00:00

Language: English

Source URL: https://arxiv.org/abs/2412.03186

Source PDF: https://arxiv.org/pdf/2412.03186

Licence: https://creativecommons.org/licenses/by/4.0/

Changes: This summary was created with assistance from AI and may have inaccuracies. For accurate information, please refer to the original source documents linked here.

Thank you to arxiv for use of its open access interoperability.

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