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Related Concept Videos

Elastic Collisions: Introduction01:00

Elastic Collisions: Introduction

An elastic collision is one that conserves both internal kinetic energy and momentum. Internal kinetic energy is the sum of the kinetic energies of the objects in a system. Truly elastic collisions can only be achieved with subatomic particles, such as electrons striking nuclei. Macroscopic collisions can be very nearly, but not quite, elastic, as some kinetic energy is always converted into other forms of energy such as heat transfer due to friction and sound. An example of a nearly...
Elastic Collisions: Case Study01:15

Elastic Collisions: Case Study

Elastic collision of a system demands conservation of both momentum and kinetic energy. To solve problems involving one-dimensional elastic collisions between two objects, the equations for conservation of momentum and conservation of internal kinetic energy can be used. For the two objects, the sum of momentum before the collision equals the total momentum after the collision. An elastic collision conserves internal kinetic energy, and so the sum of kinetic energies before the collision equals...
Collisions in Multiple Dimensions: Introduction01:05

Collisions in Multiple Dimensions: Introduction

It is far more common for collisions to occur in two dimensions; that is, the initial velocity vectors are neither parallel nor antiparallel to each other. Let's see what complications arise from this. The first idea is that momentum is a vector. Like all vectors, it can be expressed as a sum of perpendicular components (usually, though not always, an x-component and a y-component, and a z-component if necessary). Thus, when the statement of conservation of momentum is written for a problem,...
Detection of Black Holes01:10

Detection of Black Holes

Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...

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Related Experiment Video

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Setting Limits on Supersymmetry Using Simplified Models
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A quantum machine learning-based predictive analysis of CERN collision events.

Sarvapriya Tripathi1, Himanshu Upadhyay2, Jayesh Soni3

  • 1Department of Electrical and Computer Engineering, Florida International University, Miami, FL, USA. strip011@fiu.edu.

Scientific Reports
|December 12, 2025
PubMed
Summary
This summary is machine-generated.

Quantum Machine Learning (QML) models show promise for high-energy physics data analysis. While not outperforming advanced classical algorithms, Quantum Long Short-Term Memory (QLSTM) offers a viable approach, especially with simpler designs.

Keywords:
Dielectron eventsProton collisionQuantum long short-term memoryQuantum machine learningQuantum neural networkRegression

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Area of Science:

  • High-Energy Physics
  • Quantum Computing
  • Machine Learning

Background:

  • Quantum computing advancements drive exploration of quantum algorithms.
  • Quantum Machine Learning (QML) is investigated for potential advantages in data analysis.

Purpose of the Study:

  • To apply and evaluate Quantum Neural Network (QNN) and Quantum Long Short-Term Memory (QLSTM) models for regression tasks.
  • To compare the prediction accuracy and computational efficiency of QML models against classical regression methods using CERN datasets.

Main Methods:

  • Utilized two CERN datasets: Dielectron events and Proton collision.
  • Implemented and analyzed Quantum Neural Network (QNN) and Quantum Long Short-Term Memory (QLSTM) algorithms.
  • Compared QML performance against classical algorithms like CatBoost, analyzing various ansatz designs.

Main Results:

  • QML models achieved comparable accuracy to some classical methods, but advanced algorithms like CatBoost yielded superior results.
  • Increased circuit complexity in QNN and QLSTM did not significantly enhance prediction accuracy.
  • QLSTM with simpler ansatz designs showed particular promise for high-energy physics data.

Conclusions:

  • QML models, especially QLSTM, present a promising avenue for modeling high-energy physics data.
  • Balancing quantum circuit complexity with performance is crucial for effective QML application.
  • Further research on quantum hardware is necessary to ascertain the real-world applicability of these QML models.