Relativistic rocket
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2008-06-19T13:43:04Z
Icek
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/* Delta-v */ rapidity & multistaging
A '''relativistic rocket''' is any [[spacecraft]] that is travelling at a velocity close enough to [[light speed]] for [[special relativity|relativistic]] effects to become significant. What "significant" means is a matter of context, but generally speaking a velocity of at least 50% of the speed of light (0.5''c'') is required. The time dilation factor, mass factor, and length contraction factor (all these factors equal the [[Lorentz factor]]) are 1.15 at 0.5''c''. Above this speed Einstein's physics are required to describe motion. Below this speed, motion is approximately described by Newtonian physics and the [[Tsiolkovsky rocket equation]] can be used.
We define a rocket as carrying all of its reaction mass, energy, and engines with it. [[Bussard ramjet]]s, [[rair]]s,<ref>http://scientium.com/diagon_alley/commentary/bowden_essays/sotm/starship/rockets.htm#rair</ref><!--- What is a rair? nothing in wikipedia yet.--> [[light sail]]s, and [[maser]] or [[laser]]-electric vehicles are not rockets.
Achieving relativistic velocities is difficult, requiring advanced forms of [[spacecraft propulsion]] that have not yet been adequately developed. [[Nuclear pulse propulsion]] could theoretically achieve 0.1''c'' using current known technologies, but would still require many engineering advances to achieve this. The relativistic gamma factor (<math>\gamma</math>) at 10% of light velocity is 1.005. The time dilation factor of 1.005 which occurs at 10% of light velocity is too small to be of major significance. A 0.10''c'' velocity interstellar rocket is thus considered to be a non-relativistic rocket because its motion is quite accurately described by Newtonian physics alone.
Relativistic rockets are usually seen discussed in the context of [[interstellar travel]], since most would require a great deal of space to accelerate up to those velocities. They are also found in some [[thought experiment]]s such as the [[twin paradox]].
== Relativistic rocket equation ==
As with the classical rocket equation, one wants to calculate the velocity change <math>\Delta v</math> that a rocket can achieve depending on the [[specific impulse]] <math>I_{sp}</math> and the mass ratio, i. e. the ratio of starting mass <math>m_0</math> and mass at the end of the acceleration phase (dry mass) <math>m_1</math>. It should be noted that subsequently ''specific impulse'' means the momentum produced by the exhaust of a certain amount of rocket fuel divided by the mass of that amount of rocket fuel. Thus specific impulse is a velocity, as opposed to the common usage of the word as the ratio of momentum and weight (weight would not make much sense in this context).
=== Specific impulse ===
The specific impulse of relativistic rockets is the same as the effective exhaust velocity, despite the fact that the nonlinear relationship of velocity and momentum as well as the conversion of matter to energy have to be taken into account; the two effects cancel each other. Of course this is only valid if the rocket does not have an external energy source (e. g. a laser beam from a space station; in this case the momentum carried by the laser beam also has to be taken into account). If all the energy to accelerate the fuel comes from an external source (and there is no additional momentum transfer), then the relationship between effective exhaust velocity and specific impulse is as follows:
:<math>I_{sp} = \frac {v_e}{\sqrt{1 - \frac{v_e^2}{c^2}}} = \gamma \ v_e</math>
where <math>\gamma</math> is the [[Lorentz factor]]. In the case of no external energy source, the relationship between <math>I_{sp}</math> and the fraction of the fuel mass <math>\eta</math> which is converted into energy might also be of interest; assuming no losses, it is
:<math>\eta = 1 - \sqrt{1 - \frac{I_{sp}^2}{c^2}} = 1 - \frac{1}{\gamma}</math>
The inverse relation is
:<math>I_{sp} = c \cdot \sqrt{2 \eta - \eta^2}</math>
Here are some examples of fuels, the energy conversion fractions, and the specific impulses (assuming no losses if not specified otherwise):
{| class="wikitable"
!Fuel||<math>\eta</math>||<math>I_{sp} / c</math>
|-
|[[electron]]-[[positron]] annihilation
|1
|1
|-
|[[proton]]-[[antiproton]] annihilation, using only charged [[pion]]s
|0.56
|0.60
|-
|[[electron]]-[[positron]] annihilation with simple hemispherical absorption of gamma rays
|1
|0.25
|-
|[[nuclear fusion]]: [[Hydrogen|H]] to [[Helium|He]]
|0.00712
|0.119
|-
|[[nuclear fission]]: <sup>235</sup>[[Uranium|U]]
|0.001
|0.04
|}
=== Delta-v ===
In order to make the calculations simpler, we assume that the acceleration is constant (in the rocket's reference frame) during the acceleration phase; however, the result is nonetheless valid if the acceleration varies, as long as <math>I_{sp}</math> is constant.
In the nonrelativistic case, one knows from the (classical) Tsiolkovsky rocket equation that
:<math>\Delta v = I_{sp} \ln \frac {m_0}{m_1}</math>
Assuming constant acceleration <math>a</math>, the time span <math>t</math> during which the acceleration takes place is
:<math>t = \frac {I_{sp}}{a} \ln \frac {m_0}{m_1}</math>
In the relativistic case, the equation still valid if <math>a</math> is the acceleration in the rocket's reference frame and <math>t</math> is the rocket's proper time because at velocity 0 the [[Special relativity#Force|relationship between force and acceleration]] is the same as in the classical case.
By applying the [[Lorentz transformation]] on the acceleration, one can calculate the end velocity <math>\Delta v</math> relative to the rest frame (i. e. the frame of the rocket before the acceleration phase) as a function of the rocket frame acceleration and the rest frame time <math>t'</math>; the result is
:<math>\Delta v = \frac {a \cdot t'} {\sqrt{1 + \frac{(a \cdot t')^2}{c^2}}}</math>
The time in the rest frame relates to the proper time by the following equation:
:<math>t' = \frac{c}{a} \sinh \left(\frac{a \cdot t}{c} \right)</math>
Substituting the proper time from the Tsiolkovsky equation and substituting the resulting rest frame time in the expression for <math>\Delta v</math>, one gets the desired formula:
:<math>\Delta v = c \cdot \tanh \left(\frac {I_{sp}}{c} \ln \frac{m_0}{m_1} \right)</math>
The formula for the corresponding [[rapidity]] (the [[Inverse hyperbolic functions|area hyperbolic tangent]] of the velocity divided by the speed of light) is simpler:
:<math>\Delta r = \frac {I_{sp}}{c} \ln \frac{m_0}{m_1}</math>
Since rapidities, contrary to velocities, are additive, they are useful for computing the total <math>\Delta v</math> of a multistage rocket.
== Matter-antimatter annihilation rockets ==
It is clear on the basis of the above calculations that a relativistic rocket would likely need to be a rocket that is fueled by antimatter. Other antimatter rockets in addition to the photon rocket that can provide 0.5''c'' needed for interstellar space flight include the "beam core" pion rocket. In a pion rocket antimatter is stored inside [[superconducting]] electromagnetic bottles in the form of electromagnetically levitated frozen antihydrogen. Laser beams vaporize and ionize the antihydrogen a rate of a few grams per second.
The pion rocket might need a superconducting nozzle with electromagnets of 10 teslas or more. Antihydrogen and regular hydrogen are [[diamagnetic]] which allows them to be electromagnetically levitated.
=== Design notes on a pion rocket ===
{{expert}}
[[Pion]]s, also known as pi-mesons, are produced by proton-antiproton annihilation. The antiprotons will be mixed with an exactly equal mass of regular protons in the form of liquid hydrogen pumped inside the nozzle of a pion rocket engine. All of these pions have a velocity of 0.94''c'' when produced by proton-antiproton annihilation. The pions will also have a relativistic time dilation factor <math>\gamma</math> of 2.93 which extends their lifespan enough to travel 10 to 1000 meters through the nozzle, before decaying into gamma rays. Sixty percent of the pions will have either a negative, or a positive electric charge. Forty percent of the pions will be neutral. The neutral pions will decay immediately into gamma rays. Gamma rays can be reflected by some materials such as [[beryllium]]. They can also be absorbed and blocked by other materials such as [[lead]], steel, [[gold]] and uranium. The pion rocket driven starship would need a radiation shield placed between the pion rocket engine nozzle and the crew modules to protect them from the gamma rays. A [[collimator]] made of a gamma ray reflector such as [[beryllium]] metal might then be wrapped around the pion rocket nozzle.
A collimator would reflect the gamma rays into a beam at its focus, and then reflect the beam of gamma rays into space. Some additional thrust could be obtained from the radiation pressure of the reflected gamma rays on the gamma ray collimator when they are reflected by it. The charged pions would travel in helical spirals around the axial electromagnetic field lines inside the nozzle. In this way the charged pions could be collimated into an exhaust jet that is moving at 0.94''c''. This exhaust velocity is approximately 282,000,000 m/s. If 1 kg of these pions were expelled per second the pion engine would have a thrust of 282,000,000 newtons. A pion rocket will use a superconducting electromagnetic nozzle to collimate the beam of electrically-charged pions created by proton-antiproton annihilation, into a rocket exhaust jet. The property of diamagnetism, which is possessed by both hydrogen, and anti-hydrogen will be used, to store the antimatter, in the form of anti-hydrogen ice, by levitating it, in the center of an electromagnetic field, inside, a super conducting electromagnetic vacuum bottle.
== Sources ==
# ''The star flight handbook,'' Matloff & Mallove, 1989
# ''Mirror matter: pioneering antimatter physics,'' Dr. Robert L Forward, 1986
==References==
<references/>
==External links==
*[http://math.ucr.edu/home/baez/physics/Relativity/SR/rocket.html Physics FAQs: The Relativistic Rocket]
*[http://www.geocities.com/albmont/relroket.htm Javascript that calculates the Relativistic Rocket Equation]
*''Spacetime Physics: Introduction to Special Relativity'' (1992). W. H. Freeman, ISBN 0-7167-2327-1
[[Category:Interstellar travel]]
[[Category:Spacecraft propulsion]]
[[de:Interstellare Raumfahrt#Relativistischer_Flug]]
[[fr:Voyage relativiste]]