New Pulsar Emission Mechanism?

In summary, Andrea Schmidt and John Singleton of Los Alamos National Laboratory provide detailed analyses of several pieces of observational data that suggest that pulsars emit the electromagnetic equivalent of the well-known "sonic boom" from accelerating supersonic aircraft. Just as the "boom" can be very loud a long way from the aircraft, the analogous signals from the pulsar remain intense over very long distances. The superluminal group velocity caused by the neutral hydrogen in the interstellar medium means that these pulses appear to travel faster than light.
  • #1
Bob S
4,662
7
In papers presented this week to the American Astronomical Society, Andrea Schmidt and John Singleton of Los Alamos National Laboratory provide detailed analyses of several pieces of observational data that suggest that pulsars emit the electromagnetic equivalent of the well-known "sonic boom" from accelerating supersonic aircraft. Just as the "boom" can be very loud a long way from the aircraft, the analogous signals from the pulsar remain intense over very long distances.

Schmidt and Singleton's presentations provide strong support for a pulsar emission mechanism (the superluminal model) due to circulating polarization currents that travel faster than the speed of light. These superluminal polarization currents are disturbances in the pulsar's plasma atmosphere in which oppositely-charged particles are displaced by small amounts in opposite directions; they are induced by the neutron star's rotating magnetic field. Despite the large speed of the polarization current itself, the small displacements of the charged particles that make it up means that their velocities remain slower than light, so that Einstein's theory of Special Relativity is not violated. No laws of physics are broken in this model.

See
http://www.spaceref.com/news/viewpr.html?pid=29949
 
Astronomy news on Phys.org
  • #2
Sigh... I'm just waiting for this paper to be totally misinterpreted.

It should be noted that in electromagnetic waves, it is *very common* for patterns to travel faster than light. One pretty trivial example, is imagine your television screen. It's very easy to move a dot across the screen in the screen that moves faster than light.

The big no-no is to transmit information faster the light.
 
  • #3
Apparent Faster-Than-Light Pulse Propagation in Interstellar Space: A new
probe of the Interstellar Medium

ABSTRACT
"Radio pulsars emit regular bursts of radio radiation that propagate through the
interstellar medium (ISM), the tenuous gas and plasma between the stars. Previously
known dispersive properties of the ISM cause low frequency pulses to be delayed in
time with respect to high frequency ones. This effect can be explained by the presence
of free electrons in the medium. The ISM also contains neutral hydrogen which has a
well known resonance at 1420.4 MHz. Electro-magnetic theory predicts that at such
a resonance, the induced dispersive effects will be drastically different from those of
the free electrons. Pulses traveling through a cloud of neutral hydrogen should undergo
“anomalous dispersion,” which causes the group velocity of the medium to be larger than
the speed of light in vacuum. This superluminal group velocity causes pulses containing
frequencies near the resonance to arrive earlier in time with respect to other pulses.
Hence, these pulses appear to travel faster than light.
"
See http://arxiv.org/PS_cache/arxiv/pdf/0909/0909.2445v2.pdf
Bob S
 

Related to New Pulsar Emission Mechanism?

1. What is a pulsar and how does it emit radiation?

A pulsar is a highly magnetized, rapidly rotating neutron star that emits beams of electromagnetic radiation along its magnetic poles. This radiation is produced by the acceleration of charged particles within the pulsar's magnetic field.

2. What is the new pulsar emission mechanism?

The new pulsar emission mechanism is a theoretical model proposed by scientists to explain the origin of pulsar radiation. It suggests that the radiation is produced by the interaction between the pulsar's strong magnetic field and the intense plasma surrounding it.

3. How does the new mechanism differ from previous models?

The new pulsar emission mechanism differs from previous models in that it takes into account the complex interplay between the pulsar's magnetic field and the surrounding plasma. It also offers a more detailed explanation for the observed properties of pulsar radiation.

4. What evidence supports the new pulsar emission mechanism?

There is strong evidence supporting the new pulsar emission mechanism, including observations of pulsar radiation that cannot be explained by previous models. Additionally, simulations based on this mechanism have been able to accurately reproduce the observed properties of pulsars.

5. How does understanding the pulsar emission mechanism benefit scientific research?

Understanding the pulsar emission mechanism is crucial for advancing our understanding of the physical processes that occur in extreme environments. It also has practical applications, such as improving our ability to detect and study pulsars, which can serve as important probes for studying the properties of the universe.

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