Antimatter rockets would offer the highest
specific impulse of any known rocket technology and thus would most easily be able to achieve relativistic speeds, though the change of mass due to
annihilation means the above rocket equation does not hold. Other antimatter rockets in addition to the photon rocket that can provide a 0.6
c specific impulse (studied for basic
hydrogen-
antihydrogen annihilation, no
ionization, no recycling of the radiation) 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 peta
watts 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. 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.
Design notes on a pion rocket The pion rocket has been studied independently by Robert Frisbee 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 0.94
c (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. The remaining heat will also require the shield to be refrigerated. 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 0.94
c. 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. 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==