Relativistic rocket explained

Relativistic rocket means any spacecraft that travels close enough to light speed for relativistic effects to become significant. The meaning of "significant" is a matter of context, but often a threshold velocity of 30% to 50% of the speed of light (0.3c to 0.5c) is used. At 30% c, the difference between relativistic mass and rest mass is only about 5%, while at 50% it is 15%, (at 0.75c the difference is over 50%); so above such speeds special relativity is needed to accurately describe motion, while below this range Newtonian physics and the Tsiolkovsky rocket equation usually give sufficient accuracy.

In this context, a rocket is defined as an object carrying all of its reaction mass, energy, and engines with it.

\gamma at 10% of light velocity is 1.005. A 0.1c speed rocket is thus considered non-relativistic since its motion is still quite accurately described by Newtonian physics alone.

Relativistic rockets are usually seen discussed in the context of interstellar travel, since most would need a lot of space to reach such speed. They are also found in some thought experiments such as the twin paradox.

Relativistic rocket equation

As with the classical rocket equation, one wants to calculate the velocity change

\Delta v that a rocket can achieve depending on the exhaust speed v _{e} and the mass ratio, i. e. the ratio of starting rest mass m _{0} and rest mass at the end of the acceleration phase (dry mass) m _{1} .

In order to make calculations simpler, we assume that the acceleration is constant (in the rocket's reference frame) during the acceleration phase; still, the result is nonetheless valid if the acceleration varies, as long as exhaust velocity

v _{e} is constant.

In the nonrelativistic case, one knows from the (classical) Tsiolkovsky rocket equation that

\Delta v = v _{e} ln (m _{0})/(m _{1}) . Assuming constant acceleration a , the time span t during which the acceleration takes place ist = (v _{e})/(a) ln (m _{0})/(m _{1}) . In the relativistic case, the equation is still valid if a is the acceleration in the rocket's reference frame and t is the rocket's proper time because at velocity 0 the relationship between force and acceleration is the same as in the classical case. Solving this equation for the ratio of initial mass to final mass gives(m _{0})/(m _{1}) = \exp\left[ (at)/(v _{e}) \right]. where "exp" is the exponential function. Another related equation^[1] gives the mass ratio in terms of the end velocity \Delta v relative to the rest frame (i. e. the frame of the rocket before the acceleration phase):(m _{0})/(m _{1}) = \left[ (1 + { (\Delta v)/(c))/() }\right]^.For constant acceleration, (\Delta v)/(c) = \tanh\left[ (at)/(c) \right] (with a and t again measured on board the rocket),^[2] so substituting this equation into the previous one and using the hyperbolic function identity \tanh x = (e ^{2x} -1)/(e ^{2x} +1) returns the earlier equation (m _{0})/(m _{1}) = \exp\left[ (at)/(v _{e}) \right] .

By applying the Lorentz transformation, one can calculate the end velocity

\Delta v as a function of the rocket frame acceleration and the rest frame time t' ; the result is\Delta v = (a t')/(\sqrt{ 1 + ((a t') ^{2})/(c ^{2})) }.The time in the rest frame relates to the proper time by the hyperbolic motion equation:t' = (c)/(a) \sinh \left( (a t)/(c) \right). Substituting the proper time from the Tsiolkovsky equation and substituting the resulting rest frame time in the expression for \Delta v , one gets the desired formula:\Delta v = c \tanh \left( (v _{e})/(c) ln (m _{0})/(m _{1}) \right). The formula for the corresponding rapidity (the inverse hyperbolic tangent of the velocity divided by the speed of light) is simpler:\Delta r = (v _{e})/(c) ln (m _{0})/(m _{1}) . Since rapidities, contrary to velocities, are additive, they are useful for computing the total \Delta v of a multistage rocket.

Matter-antimatter annihilation rockets

It is clear from the above calculations that a relativistic rocket would likely need to be antimatter-fired. Other antimatter rockets in addition to the photon rocket that can provide a 0.6c specific impulse (studied for basic hydrogen-antihydrogen annihilation, no ionization, no recycling of the radiation^[3]) needed for interstellar flight include the "beam core" pion rocket. In a pion rocket, frozen antihydrogen is stored inside electromagnetic bottles. Antihydrogen, like regular hydrogen, is diamagnetic which allows it to be electromagnetically levitated when refrigerated. Temperature control of the storage volume is used to determine the rate of vaporization of the frozen antihydrogen, up to a few grams per second (hence several petawatts when annihilated with equal amounts of matter). It is then ionized into antiprotons which can be electromagnetically accelerated into the reaction chamber. The positrons are usually discarded since their annihilation only produces harmful gamma rays with negligible effect on thrust. However, non-relativistic rockets may exclusively rely on these gamma rays for propulsion.^[4] This process is necessary because un-neutralized antiprotons repel one another, limiting the number that may be stored with current technology to less than a trillion.^[5]

Design notes on a pion rocket

The pion rocket has been studied independently by Robert Frisbee^[6] and Ulrich Walter, with similar results. Pions, short for pi-mesons, are produced by proton-antiproton annihilation. The antihydrogen or the antiprotons extracted from it will be mixed with a mass of regular protons pumped into the magnetic confinement nozzle of a pion rocket engine, usually as part of hydrogen atoms. The resulting charged pions have a speed of 0.94c (i.e.

\beta = 0.94), and a Lorentz factor \gamma of 2.93 which extends their lifespan enough to travel 21 meters through the nozzle before decaying into muons. 60% of the pions will have either a negative, or a positive electric charge. 40% of the pions will be neutral. The neutral pions decay immediately into gamma rays. These can't be reflected by any known material at the energies involved, though they can undergo Compton scattering. They can be absorbed efficiently by a shield of tungsten placed between the pion rocket engine reaction volume and the crew modules and various electromagnets to protect them from the gamma rays. The consequent heating of the shield will make it radiate visible light, which could then be collimated to increase the rocket's specific impulse.^[3] The remaining heat will also require the shield to be refrigerated.^[6] The charged pions would travel in helical spirals around the axial electromagnetic field lines inside the nozzle and in this way the charged pions could be collimated into an exhaust jet moving at 0.94c. In realistic matter/antimatter reactions, this jet only represents a fraction of the reaction's mass-energy: over 60% of it is lost as gamma-rays, collimation is not perfect, and some pions are not reflected backward by the nozzle. Thus, the effective exhaust speed for the entire reaction drops to just 0.58c.^[3] Alternate propulsion schemes include physical confinement of hydrogen atoms in an antiproton and pion-transparent beryllium reaction chamber with collimation of the reaction products achieved with a single external electromagnet; see Project Valkyrie.

See also

• Rocket propulsion technologies (disambiguation)

Sources

• The star flight handbook, Matloff & Mallove, 1989. Also See on the Bussard ramjet page, under the related inventions section.
• Mirror matter: pioneering antimatter physics, Dr. Robert L Forward, 1986

External links

• Physics FAQs: The Relativistic Rocket
• Javascript that calculates the Relativistic Rocket Equation
• Spacetime Physics: Introduction to Special Relativity (1992). W. H. Freeman,
• The Relativistic Photon Rocket

Notes and References

1. Forward, Robert L. "A Transparent Derivation of the Relativistic Rocket Equation" (see the right side of equation 15 on the last page, with R as the ratio of initial to final mass and w as the specific impulse)
2. Web site: The Relativistic Rocket . Math.ucr.edu . 2015-06-21.
3. 0910.1965. Westmoreland. Shawn. A note on relativistic rocketry. Acta Astronautica. 67. 9–10. 1248–1251. 2009. 10.1016/j.actaastro.2010.06.050. 2010AcAau..67.1248W. 54735356 .
4. Web site: New Antimatter Engine Design. 29 October 2006 .
5. Web site: Reaching for the Stars - NASA Science . Science.nasa.gov . 2015-06-21.
6. Web site: How to Build an Anitmatter Rocket for Interstellar Missions . Relativitycalculator.com . 2015-06-21.