Encounters with Modern Physics | Prof. Samuel C.C. Ting

Encounters with Modern Physics | Prof. Samuel C.C. Ting

Welcome and Introduction

Opening Remarks

  • The speaker expresses pleasure in welcoming Professor Ting, who joins online due to other commitments.
  • The event is the 22nd special public lecture, indicating its significance.

Audience Engagement

Interaction with Viewers

  • Audience members are encouraged to post questions in the chat box during the lecture for later discussion.

Professor Ting's Lecture Topic

Overview of Presentation

  • Professor Ting introduces his talk on "Encounters with Modern Physics," sharing personal experiences from five decades of experiments.

Historical Context: Cosmic Rays

Significance of Cosmic Rays

  • This year marks the 125th anniversary of Manuel Bhabha's contributions to cosmic ray research, highlighting his role in explaining latitude development and intensity through the famous Lamat Bhabha Theory.
  • Bhabha completed his PhD at MIT in 1924 and mentored notable physicists like Richard Feynman.

Development of Accelerators

Evolution Over Centuries

  • Accelerators have evolved over 400 years; the largest ground accelerator today is a 27 km proton collider used for studying fundamental particles.

First Encounter with Particle Physics

Measuring Electron Size

  • Professor Ting recounts his first experiment aimed at measuring electron size, which was based on modern electromagnetic theory suggesting electrons have zero radius.

Harvard-MIT Experiment Insights

Key Findings from Experiments

  • A significant measurement conducted by Harvard and MIT challenged existing theories by showing deviations from quantum electrodynamics at small distances (10^-13 cm to 10^-14 cm).

Independent Confirmation of Results

Pursuing Further Research

  • Following initial findings, Professor Ting sought independent verification through an experiment he led after moving to Germany, despite lacking prior experience in electron physics.

Hamburg Accelerator Experience

Experimental Setup Description

  • At Hamburg’s electron accelerator, innovative designs were employed including using dipole magnets and multiple counters for precise measurements amidst high background noise levels.

Experiment Outcomes and Discoveries

Conclusion of Findings

Experimental Physics Insights

Announcement of Results and Key Collaborations

  • The results were first announced in 1965 at the Rochester conference, now known as the International Conference on High Energy Physics. Important figures met during this event included Panovski, Fan, and Robbie.
  • The initial paper published focused on validating quantum electrodynamics (QED) at small distances, with contributions from colleagues at Columbia University.

Lessons Learned in Experimental Physics

  • A critical lesson learned is to not always accept expert results blindly; even world-class experts can have discrepancies in measurements.
  • Observations showed deviations from QED when measuring electron-positron pairs' invariant mass, particularly notable at 700 GeV and 1 GeV due to massive particle transformations.

Photon Interactions and Vector Dominance Model

  • Heavy photons (massive particles like rho and omega mesons) share quantum numbers with regular photons but differ in mass. This leads to significant implications for high-energy interactions.
  • The interaction model suggests that photons interacting with nuclei can be replaced by heavy photon interactions under certain conditions, leading to a deeper understanding of particle behavior.

Precision Experiments at MIT

  • After joining MIT, advancements were made in detector precision for better coordinate resolution and particle identification.
  • An example of coherent interference patterns between rho and omega decays was observed, highlighting differences in scattering behaviors based on final states.

Challenges in Experimental Observations

  • Despite predictions of certain interactions existing involving alpha to the third order, experimental evidence remained elusive due to low branching ratios making detection difficult.
  • Data indicated that only rho and omega interference could explain certain measurements accurately; other models failed to align with observed data.

New Forms of Matter Exploration

  • Research revealed that photons can transform into heavy photons under specific conditions. This led to experiments aimed at discovering new forms of matter using high-intensity fluxes.
  • A proposal was made for an experiment at Brookhaven National Laboratory focusing on vector meson production through proton-proton collisions.

Methodological Considerations for Future Experiments

  • Emphasis was placed on using high-duty cycle extracted beams for efficient experimentation while avoiding angular distribution measurement complexities inherent in e+e− storage rings.
  • The discussion highlighted the importance of systematic searches for heavy mesons through continuous energy variation rather than relying solely on fixed energy points.

Experimental Challenges in Particle Physics

Overview of the Brook Experiment

  • The Brook experiment aims to observe rare electron-positron pairs, requiring significant adjustments to the accelerator's orbit.
  • Observing these pairs is extremely challenging, with a detection rate of less than 10^8, necessitating a rejection factor of 10^10.
  • The physics community largely dismissed the search for heavy photons as uninteresting, leading to initial rejections of the experimental proposal.

Acceptance and Design of the Experiment

  • Eventually, Brookhaven National Laboratory accepted the proposal; an overview of the experimental layout was provided.
  • The design includes various components such as magnets and detectors aimed at measuring momentum and angles for optimal mass resolution.

Instrumentation and Detection Techniques

  • A T cup counter was developed to achieve a rejection rate of 10^10; hydrogen gas was chosen despite its low photon production due to safety concerns.
  • A position detector designed by UIC Beer utilized geometric principles to differentiate signals from background noise.

Radiation Protection Measures

  • To manage radiation from high particle collisions (10^12 protons), substantial shielding materials were employed: concrete, uranium, lead, and salt were used strategically.

Initial Findings and Observations

  • Early data indicated a sharp peak at 3.1 GeV in electron-positron mass measurements; further tests confirmed this observation under varying magnetic fields.
  • The production rate of J particles increased significantly with energy levels across different laboratories.

Significance of Discoveries

  • The J particle exhibited an exceptionally long lifetime (10,000 times longer than other particles), suggesting unique properties akin to discovering extraordinary longevity in living organisms.
  • Continued research over decades led to new findings about exotic particles formed through gluon interactions.

Lessons Learned from Experimental Challenges

Discovery of Gluon and Particle Physics Experiments

Understanding the Role of Gluons

  • The discovery of gluons is crucial in understanding atomic structure, where protons and neutrons are composed of quarks held together by the strong force known as GL.

Positron-Electron Collider Experiment

  • The positron-electron collider in Hamburg, Germany, was designed to verify newly formed electroweak theory through experiments like the MAR experiment, which measured forward-backward asymmetry.

Observations from Electron-Positron Collisions

  • Data from electron-positron collisions indicated the existence of virtual Z bosons, confirming electroweak theory while showing discrepancies with quantum chromodynamics (QCD).

Jet Production and Gluon Energy

  • When gluon energy increases during collisions, three jets are produced instead of two. This phenomenon can be explained by considering quark-antiquark pairs with large momentum transfer.

Statistical Significance in Experimental Results

  • The observation of three jets is significant; however, it requires sufficient statistical events to validate against the quark-gluon model. This was highlighted in findings published in Physical Review Letters.

Long-Term Collaborations and Technological Advances

Importance of International Collaboration

  • Over 21 years, a collaboration involving 20 countries aimed to explore fundamental particles using a high-energy positron-electron collider at unprecedented temperatures.

Technical Innovations for Experiments

  • A major technical achievement was producing B crystals necessary for accurate measurements. Initially thought impossible, 12 tons were produced within three years for the L3 experiment.

Outcomes and Contributions to Physics

  • The extensive research led to over 300 published papers and PhD degrees awarded. Key findings included identifying only three types of electrons and establishing limits on particle sizes.

Lessons Learned from Particle Physics Research

Agreement with Current Theories

  • Most experimental results aligned well with existing theories on elementary particles; however, they offered limited new insights due to this agreement.

Value of Large International Collaborations

  • Successful collaborations require selecting important topics that engage scientists across diverse backgrounds while ensuring recognition for young researchers involved.

Future Directions: Space-Based Experiments

Exploring Fundamental Science via ISS

  • Current projects involve international cooperation on fundamental science aboard the International Space Station (ISS), which serves as an advanced laboratory for high-energy particle physics research.

Fundamental Discoveries in Modern Physics

Key Discoveries and Experiments

  • The foundation of modern physics includes significant discoveries such as the positron, cosmic neutrinos, and charge-mass ratios before high-energy accelerators were developed.
  • Notable cosmic ray experiments are conducted globally, including locations like Mexico, Tibet (4.4 km above sea level), and Argentina, alongside the IceCube experiment at the South Pole.
  • The passing of Edward Stone is acknowledged; he was a pioneer in cosmic exploration with Voyager 1 and Voyager 2. His contributions to physics are greatly missed.

Cosmic Ray Studies

  • Research focuses on dark matter, antimatter, and cosmic origins through precision measurements of cosmic rays that penetrate Earth's atmosphere.
  • Collaboration among international scientists is emphasized; none have prior experience conducting space experiments.

Advanced Detection Techniques

Spectrometer Design

  • A spectrometer utilizes transition radiation detectors to identify electrons and positrons while measuring their momentum and charge using silicon trackers.
  • The experimental setup includes multiple layers for particle detection: upper time-of-flight counters measure direction while electromagnetic counters assess energy.

Data Collection Timeline

  • Continuous data collection from the space station is planned from 2011 until 2025, with an extension to enhance detection capabilities by adding more silicon trackers.

Recent Findings on Cosmic Particles

Particle Origins

  • Recent measurements indicate that particles can originate from various sources including dark matter interactions or collisions involving protons.
  • Analysis of over 4.2 million events reveals distinct energy distributions between low-energy cosmic rays (from standard calculations) and high-energy events potentially linked to new sources.

Spectrum Analysis

  • Latest spectral data shows a correlation between cosmic radiation models and dark matter interactions; however, uncertainties remain evident in measurement accuracy.

Understanding Cosmic Rays' Composition

Antiproton Observations

  • Observations show that antiproton-to-proton ratios become energy-independent above 60 GeV; this suggests unique production mechanisms for these particles.

Primary vs Secondary Cosmic Rays

  • Primary cosmic rays are formed during stellar lifetimes and accelerated by supernovae; understanding their propagation is crucial for astrophysics.

Elemental Abundance Insights

Elemental Measurements

Understanding the Role of Carbon and Boron in Cosmic Models

The Distinction Between Primary and Secondary Elements

  • Discussion on the characteristics of elements like Boron, Florin, and Scandium as secondary elements compared to primary ones. The longstanding idea is that carbon is considered a pure primary element while Boron is viewed as purely secondary.
  • Findings indicate that carbon is not purely primary; it has a significant secondary component. This raises questions about the relevance of using Boron over carbon in cosmological models.

Composition Analysis of Elements

  • Overview of the primary and secondary compositions of various elements including hydrogen, helium, lithium, boron, carbon, and sulfur. Most elements fall between pure primary and pure secondary categories.
  • Measurement results show 21 out of 28 elements have been analyzed for their isotopic composition, revealing four distinct groups based on their primary and secondary classifications.

Isotope Measurements and Their Implications

  • Explanation of how momentum (p) and velocity (v) measurements are used to determine mass (M). Techniques include using spectrometers for momentum measurement and time-of-flight counters for velocity.
  • Recent findings suggest that cosmic deuterium (D), previously thought to be solely a secondary particle, actually has a significant primary component.

Antimatter Research Insights

  • Introduction to heavy antimatter where matter is defined by its mass (m) and charge (Z). Antimatter particles mirror these properties but with opposite charges.
  • Description of detecting anti-deuterons using precision spectrometers like AMS. A specific anti-deuteron candidate was identified among millions of protons.

Experimental Challenges and Curiosity in Research

  • After 12 years of data collection, statistics reveal numerous events related to matter electrons versus antimatter positrons. The search continues for candidates like anti-carbon.
  • Emphasis on the importance of curiosity in experimental physics. Researchers are encouraged to enjoy their work while striving towards achieving their goals.

Questions from the Audience

  • Clarification regarding the use of soap instead of heavy metals in experiments due to its effectiveness in absorbing neutrons through its high water content.
  • Discussion about expected rates for antimatter candidates such as anti-helium being significantly higher than conventional predictions—10 million times higher than expected rates.

The Scientific Implications of the Discovery of J Meon

Overview of the Nobel Prize Recognition

  • The speaker discusses the scientific implications of discovering J Meon, which led to a Nobel Prize awarded two years later. The citation highlighted that both researchers discovered a new form of matter.

Brookhaven's Acceptance of the Proposal

  • A question arises about why Brookhaven accepted a proposal for an experiment that other labs turned down. The speaker admits uncertainty but notes that at the time, there was no established theory or model for cork interactions, making it seem unfeasible.

Data Analysis in Experiments

  • A colleague from India asks about data analysis priorities—whether to focus on self-acquired data or Monte Carlo simulations. The speaker emphasizes that both are essential for accurate analysis and understanding acceptance rates.

Production Challenges in Particle Physics

  • Before the L3 experiment, global production of Bjo was only 4 kg per year; however, L3 required 12 tons. The speaker attributes this significant increase to support from the Soviet Union and addressing supply chain issues rather than personal achievement.

Journey into Particle Physics

  • Initially studying mechanical engineering at Michigan University, the speaker switched to physics and mathematics after struggling with engineering concepts. Encouraged by his advisor, he pursued experimental physics due to its practical applications and importance in measurement.

Influence of Mentorship on Career Path

  • Working with renowned physicist Ulen influenced the speaker’s decision to become an experimentalist over a theorist. Ulen noted that average experimentalists contribute significantly through measurements compared to theoretical counterparts.

Observations on Secondary Particles

  • A general question is raised regarding why secondary particles depend strongly on rigidity. The speaker admits a lack of explanation but acknowledges it as an observed fact without current theoretical backing.

Conference Engagement and Audience Appreciation

  • During a conference attended by around 100 people across various locations, questions were gathered from streaming platforms like YouTube and Facebook. The session concludes with expressions of gratitude towards the speaker for their inspiring talk and valuable lessons shared.
Video description

An interesting aspect of this conference was that Professor Ting made it unique and special for ISVHECRI 2024, recounting his experiences and sharing fundamental lessons for young students and scientists in STEM fields (Science, Technology, Engineering, and Mathematics). Although he had to cancel his physical assistance due to work commitments and at the last moment he agreed to give the conference online with the support of the Data Analysis and Supercomputing Center (CADS, UdeG) and the University Corporation for Internet Development (CUDI). Professor Ting's participation in ISVHECRI 2024 and his first appearance in Jalisco were made possible thanks to the efforts of the International Advisory Committee President, Professor Sunil Gupta, and the Local Organizing Committee President, Doctor Eduardo de la Fuente Acosta. According to UdeG (2024) Professor Ting during his conference recommended six lessons for young scientists: 1. Do not always accept the results of experts. 2. For an experimental scientist, precision instrumentation with redundancy is vital. 3. Maintain faith in yourself and do what you believe is right. 4. Be prepared for surprises in experimental results. 5. Large international collaborations are essential in many areas of fundamental research. To succeed, it is necessary to: - Choose an important topic. - Recognize young scientists. - Respect the diversity of all collaborators. - Not compromise the instrumentation and build the best possible detector. 6. Be curious, enjoy what you do, and work hard to achieve your goals. The video of the live conference is available at the following link: Red Cudi México. (11 de julio del 2024). Encounters with Modern Physics. [Archivo de video]. YouTube. https://www.youtube.com/watch?v=-vQwLF9kLbM. ------------------------------------------------------------------------------------------------------------- Un aspecto interesante de esta presentación fue que el Profesor Ting la hizo única y especial para el ISVHECRI 2024, relatando sus experiencias y compartiendo lecciones fundamentales para jóvenes estudiantes y científicos en áreas STEM (Ciencia, Tecnología, Ingeniería y Matemáticas). Aunque tuvo que cancelar su presencia física por cuestiones de trabajo y de ultimo momento aceptó dar la conferencia en línea con el apoyo del Centro de Análisis de Datos y Supercómputo (CADS, UdeG) y la Corporación Universitaria para el Desarrollo de Internet (CUDI). La participación del Profesor Ting en el ISVHECRI 2024 y en Jalisco por primera vez se logró gracias a la gestión de los presidentes del Comité Asesor Internacional y del Comité Organizador Local del ISVHECRI 2024, Profesor Sunil Gupta y Doctor Eduardo de la Fuente Acosta, respectivamente. De acuerdo con la UdeG (2024) el profesor Ting mencionó las siguientes lecciones para los jóvenes científicos durante su conferencia: 1. No acepte siempre los resultados de los expertos. 2. Para un científico experimental, la instrumentación de precisión con redundancia es vital. 3. Mantenga la fe en sí mismo y haga lo que crea correcto. 4. Esté preparado para sorpresas en los resultados experimentales. 5. Las grandes colaboraciones internacionales son esenciales en muchas áreas de la investigación fundamental. Para tener éxito, es necesario: - Elegir un tema importante. - Reconocer al joven científico. - Respetar la diversidad de todos los colaboradores. - No comprometer la instrumentación y construir el mejor detector posible. 6. Sea curioso, disfrute lo que hace y trabaje duro para lograr sus objetivos. El video de la conferencia en directo está disponible en la siguiente liga: Red Cudi México. (11 de julio del 2024). Encounters with Modern Physics. [Archivo de video]. YouTube. https://www.youtube.com/watch?v=-vQwLF9kLbM. ------------------------------------------------------------------------------------------------------- Referencias / References: - Universidad de Guadalajara. (2024). Memorias y Lecciones de un Premio Nobel en Física en el ISVHECRI 2024 hacia el STEM. https://www.cucei.udg.mx/es/noticia/memorias-y-lecciones-de-un-premio-nobel-en-fisica-en-el-isvhecri-2024-hacia-el-stem - Indico. (11 de julio, 2024). Encounters with Modern Physics (Encuentros con la Física Moderna). https://indico.cern.ch/event/1323265/page/34965-public-lecture-by-prof-samuel-cc-ting