Related Experiment Video
Updated: Jul 7, 2026

07:46
Setting Limits on Supersymmetry Using Simplified Models
Published on: November 15, 2013
Astrophysical bounds on photons escaping into extra dimensions
1Elementary Particles and Field Theory Group, MS B285, Los Alamos National Laboratory, Los Alamos, NM 87545, USA.
Physical Review Letters
|February 1, 2008
Summary
In extra-dimensional models, photons may escape into other dimensions. This study reveals photons in plasma are metastable, offering new bounds on these theories beyond current experiments.
Area of Science:
- Theoretical physics
- Particle physics
- Cosmology
Background:
- Extra-dimensional models with warped metrics propose gravity can localize photons on a brane.
- A key feature is the potential for photons to escape into extra dimensions.
- This phenomenon motivates precision ortho-positronium decay experiments.
Purpose of the Study:
- To investigate the implications of photons escaping into extra dimensions within a specific theoretical framework.
- To explore the metastability of photons in plasma under these conditions.
- To derive new constraints on extra-dimensional models.
Main Methods:
- Analysis of extra-dimensional models with a warped metric and a single brane.
- Theoretical investigation of photon behavior in plasma within this framework.
- Derivation of model parameter bounds based on astrophysical phenomena.
Main Results:
- Photons in plasma are predicted to be metastable in these extra-dimensional models.
- This metastability has significant implications for astrophysical cooling processes.
- New bounds derived for the model parameter far exceed the reach of current ortho-positronium experiments.
Conclusions:
- The metastability of photons in plasma provides a powerful new avenue for constraining extra-dimensional theories.
- Astrophysical observations offer significantly stronger bounds than dedicated particle physics experiments.
- These findings highlight the importance of considering astrophysical implications for fundamental physics models.
Related Concept Videos
Schwarzschild Radius and Event Horizon
No object with a finite mass can travel faster than the speed of light in a vacuum. This fact has an interesting consequence in the domain of extremely high gravitational fields.
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape velocity with the...
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape velocity with the...
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...
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...
Space-Time Curvature and the General Theory of Relativity
In 1905, Albert Einstein published his special theory of relativity. According to this theory, no matter in the universe can attain a speed greater than the speed of light in a vacuum, which thus serves as the speed limit of the universe.
This has been verified in many experiments. However, space and time are no longer absolute. Two observers moving relative to one another do not agree on the length of objects or the passage of time. The mechanics of objects based on Newton's laws of motion,...
This has been verified in many experiments. However, space and time are no longer absolute. Two observers moving relative to one another do not agree on the length of objects or the passage of time. The mechanics of objects based on Newton's laws of motion,...
Dual Nature of Electromagnetic (EM) Radiation
Electromagnetic (EM) radiation consists of electric and magnetic field components oscillating in planes perpendicular to each other and mutually perpendicular to radiation propagation through space. EM radiation can be classified as a wave, characterized by the properties of waves such as wavelength (denoted as λ) and frequency (represented by ν).
Wavelength is the distance between two consecutive peaks (the highest point) or troughs (the lowest point) in the wave. Frequency is the number of...
Wavelength is the distance between two consecutive peaks (the highest point) or troughs (the lowest point) in the wave. Frequency is the number of...
Limits of the First Law of Thermodynamics
Spontaneous processes, like a rock falling to the ground or sodium reacting with chlorine, occur without external work and often involve a decrease in the system‘s energy. However, certain endothermic processes, such as the dissolution of sodium chloride in water, occur spontaneously even though they increase the energy of the system. This limitation suggests that the First Law of Thermodynamics, which states that the total energy of a system is constant in an isolated system, cannot fully...
The de Broglie Wavelength
In the macroscopic world, objects that are large enough to be seen by the naked eye follow the rules of classical physics. A billiard ball moving on a table will behave like a particle; it will continue traveling in a straight line unless it collides with another ball, or it is acted on by some other force, such as friction. The ball has a well-defined position and velocity or well-defined momentum, p = mv, which is defined by mass m and velocity v at any given moment. This is the typical...

