Jove
Visualize
Contact Us

Related Concept Videos

Types of Radioactivity03:23

Types of Radioactivity

16.6K
The most common types of radioactivity are α decay, β decay, γ decay, neutron emission, and electron capture.
Alpha (α) decay is the emission of an α particle from the nucleus. For example, polonium-210 undergoes α decay:
16.6K
Absorption of Radiation01:05

Absorption of Radiation

706
The rate of heat transfer by emitted radiation is described by the Stefan-Boltzmann law of radiation:
706
Atomic Radii and Effective Nuclear Charge03:08

Atomic Radii and Effective Nuclear Charge

51.3K
The elements in groups of the periodic table exhibit similar chemical behavior. This similarity occurs because the members of a group have the same number and distribution of electrons in their valence shells.
51.3K
Radioactivity and Nuclear Equations03:18

Radioactivity and Nuclear Equations

20.9K
Nuclear chemistry is the study of reactions that involve changes in nuclear structure. The nucleus of an atom is composed of protons and, except for hydrogen, neutrons. The number of protons in the nucleus is called the atomic number (Z) of the element, and the sum of the number of protons and the number of neutrons is the mass number (A). Atoms with the same atomic number but different mass numbers are isotopes of the same element.
A nuclide of an element has a specific number of protons and...
20.9K
Atomic Nuclei: Nuclear Relaxation Processes01:23

Atomic Nuclei: Nuclear Relaxation Processes

622
In the absence of an external magnetic field, nuclear spin states are degenerate and randomly oriented. When a magnetic field is applied, the spins begin to precess and orient themselves along (lower energy) or against (higher energy) the direction of the field. At equilibrium, a slight excess population of spins exists in the lower energy state. Because the direction of the magnetic field is fixed as the z-axis,  the precessing magnetic moments are randomly oriented around the z-axis.
622
Atomic Nuclei: Nuclear Spin State Population Distribution01:14

Atomic Nuclei: Nuclear Spin State Population Distribution

940
Near absolute zero temperatures, in the presence of a magnetic field, the majority of nuclei prefer the lower energy spin-up state to the higher energy spin-down state. As temperatures increase, the energy from thermal collisions distributes the spins more equally between the two states. The Boltzmann distribution equation gives the ratio of the number of spins predicted in the spin −½ (N−) and spin +½ (N+) states.
940

You might also read

Related Articles

Articles linked to this work by shared authors, journal, and citation graph.

Sort by
Same author

Electronic health records: managerial insights from an umbrella review.

BMC health services research·2026
Same author

Nucleon Electric Dipole Moments in Paramagnetic Molecules through Effective Field Theory.

Physical review letters·2026
Same author

Light New Physics and the τ Lepton Dipole Moments: Prospects at Belle II.

Physical review letters·2026
Same author

Improved Calculation of Radiative Corrections to τ→ππν_{τ} Decays.

Physical review letters·2026
Same author

Elective genomic screening: results of the implementation of a whole genome sequencing program at a medical check-up unit in Spain.

Frontiers in genetics·2026
Same author

The nucleardatapy toolkit for simple access to experimental nuclear data, astrophysical observations, and theoretical predictions.

The European physical journal. A, Hadrons and nuclei·2026
JoVE
x logofacebook logolinkedin logoyoutube logo
ABOUT JoVE
OverviewLeadershipBlogJoVE Help Center
AUTHORS
Publishing ProcessEditorial BoardScope & PoliciesPeer ReviewFAQSubmit
LIBRARIANS
TestimonialsSubscriptionsAccessResourcesLibrary Advisory BoardFAQ
RESEARCH
JoVE JournalMethods CollectionsJoVE Encyclopedia of ExperimentsArchive
EDUCATION
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab ManualFaculty Resource CenterFaculty Site
Terms & Conditions of Use
Privacy Policy
Policies

Related Experiment Video

Updated: Jun 5, 2025

Setting Limits on Supersymmetry Using Simplified Models
07:46

Setting Limits on Supersymmetry Using Simplified Models

Published on: November 15, 2013

8.5K

Radiative Corrections to Superallowed β Decays in Effective Field Theory.

Vincenzo Cirigliano1, Wouter Dekens1, Jordy de Vries2,3

  • 1Institute for Nuclear Theory, <a href="https://ror.org/00cvxb145">University of Washington</a>, Seattle, Washington 91195-1550, USA.

Physical Review Letters
|December 6, 2024
PubMed
Summary

Determining the V_{ud} value requires precise radiative corrections. This study introduces an effective field theory (EFT) approach to calculate nucleus-dependent corrections (δ_{NS}), addressing a key uncertainty in V_{ud} calculations.

More Related Videos

Characterization of Recombination Effects in a Liquid Ionization Chamber Used for the Dosimetry of a Radiosurgical Accelerator
07:31

Characterization of Recombination Effects in a Liquid Ionization Chamber Used for the Dosimetry of a Radiosurgical Accelerator

Published on: May 9, 2014

11.8K
Preparing an Isotopically Pure 229Th Ion Beam for Studies of 229mTh
10:42

Preparing an Isotopically Pure 229Th Ion Beam for Studies of 229mTh

Published on: May 3, 2019

6.6K

Related Experiment Videos

Last Updated: Jun 5, 2025

Setting Limits on Supersymmetry Using Simplified Models
07:46

Setting Limits on Supersymmetry Using Simplified Models

Published on: November 15, 2013

8.5K
Characterization of Recombination Effects in a Liquid Ionization Chamber Used for the Dosimetry of a Radiosurgical Accelerator
07:31

Characterization of Recombination Effects in a Liquid Ionization Chamber Used for the Dosimetry of a Radiosurgical Accelerator

Published on: May 9, 2014

11.8K
Preparing an Isotopically Pure 229Th Ion Beam for Studies of 229mTh
10:42

Preparing an Isotopically Pure 229Th Ion Beam for Studies of 229mTh

Published on: May 3, 2019

6.6K

Area of Science:

  • Nuclear Physics
  • Particle Physics
  • Quantum Field Theory

Background:

  • Accurate determination of V_{ud} is crucial for the Standard Model.
  • Superallowed β decays are a primary source for V_{ud} values.
  • Radiative corrections, particularly nucleus-dependent ones (δ_{NS}), limit V_{ud} precision.

Purpose of the Study:

  • To develop a theoretical framework for calculating nucleus-dependent radiative corrections (δ_{NS}).
  • To utilize effective field theory (EFT) to constrain δ_{NS} and improve V_{ud} accuracy.
  • To compare EFT predictions with dispersive representations of δ_{NS}.

Main Methods:

  • Application of effective field theory (EFT) to calculate δ_{NS}.
  • Identification of dominant terms in the EFT expansion.
  • Comparison of EFT results with dispersive calculations of δ_{NS}.

Main Results:

  • The EFT power counting successfully predicts the dominant contributions to δ_{NS}.
  • The momentum scaling of δ_{NS} is observed to hold even for low-lying intermediate states.
  • A clear path towards ab initio calculations of δ_{NS} is established.

Conclusions:

  • The proposed EFT framework offers a rigorous method to calculate δ_{NS}.
  • This approach directly tackles the main uncertainty in V_{ud} determinations.
  • The study advances the precision of fundamental parameters in the Standard Model.