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module RelativityModule where
import ManifoldGeometry
import GHC.Generics (Generic)
-- βββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββ
-- Relativity: Time Dilation & Coordinate Transforms
-- βββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββ
-- | Relativity field (observer-dependent time + light cones)
data RelativityField = RelativityField
{ relativityFieldId :: String
, relativityTimeDilation :: Vector -> Double -- Returns factor < 1 near gravity
, localSpeedOfLight :: Double -- Default 299792458 m/s
, gravitationalTimeWarp :: Double -> Double -- f(potential) -> time dilation
, schwarzschildRadius :: Double -- For event horizon
} deriving (Generic)
instance Show RelativityField where
show r = "RelativityField {id=" ++ relativityFieldId r ++ "}"
-- βββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββ
-- Time Dilation
-- βββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββ
-- | Local proper time: dΟ = β(1 - vΒ²/cΒ²) β(1 - 2GM/rcΒ²) dt
-- (Schwarzschild metric with velocity)
localProperTime :: RelativityField -> Vector -> Double -> Double -> Double
localProperTime field pos velocity globalTime =
let c = localSpeedOfLight field
-- Gravitational time dilation: β(1 - Rs/r)
gravDilation = relativityTimeDilation field pos
-- Kinetic time dilation: β(1 - vΒ²/cΒ²)
beta = velocity / c
beta_clamped = min 0.9999 (abs beta) -- Clamp to avoid negative sqrt
kineticDilation = sqrt (1.0 - beta_clamped * beta_clamped)
-- Total: Ο = dt * g_tt where g_tt combines both effects
in globalTime * gravDilation * kineticDilation
-- | Gravitational potential time dilation
-- Near Schwarzschild: 1 - 2GM/(rcΒ²) = 1 - Rs/r
schwarzschildTimeDilation :: Double -> Double -> Double -> Double
schwarzschildTimeDilation rs r c =
sqrt (max 0.0001 (1.0 - rs / r)) -- Clamp to avoid negative sqrt
-- βββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββ
-- Coordinate Transformations (Special Relativity)
-- βββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββ
-- | Lorentz transformation (special relativity boost along x-axis)
-- x' = Ξ³(x - Ξ²ct)
-- t' = Ξ³(t - Ξ²x/c)
-- where Ξ³ = 1/β(1 - Ξ²Β²), Ξ² = v/c
lorentzBoostX :: Double -> Vector -> Vector
lorentzBoostX velocity pos@(Vector coords) =
let c = 299792458.0
beta = velocity / c
beta_clamped = min 0.9999 (abs beta)
gamma = 1.0 / sqrt (1.0 - beta_clamped * beta_clamped)
-- Assume coords = [ct, x, y, z]
ct = if length coords > 0 then coords !! 0 else 0
x = if length coords > 1 then coords !! 1 else 0
y = if length coords > 2 then coords !! 2 else 0
z = if length coords > 3 then coords !! 3 else 0
ct' = gamma * (ct - beta_clamped * x)
x' = gamma * (x - beta_clamped * ct)
y' = y
z' = z
in Vector [ct', x', y', z']
-- | Inverse Lorentz boost
lorentzBoostXInverse :: Double -> Vector -> Vector
lorentzBoostXInverse velocity = lorentzBoostX (-velocity)
-- | General velocity boost (along arbitrary direction)
lorentzBoost :: Vector -> Vector -> Vector
lorentzBoost velocity pos =
let c = 299792458.0
v_mag = vectorNorm velocity
beta = v_mag / c
beta_clamped = min 0.9999 (abs beta)
in if beta_clamped < 0.001
then pos -- Newtonian limit
else lorentzBoostX v_mag pos
-- βββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββ
-- Spacetime Intervals
-- βββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββ
-- | Spacetime interval (invariant)
-- sΒ² = -(cΞt)Β² + ΞxΒ² + ΞyΒ² + ΞzΒ² (signature: -+++)
spacetimeInterval :: Vector -> Vector -> Double
spacetimeInterval (Vector p1) (Vector p2) =
let dt = if length p1 > 0 && length p2 > 0 then p1 !! 0 - p2 !! 0 else 0
dx = if length p1 > 1 && length p2 > 1 then p1 !! 1 - p2 !! 1 else 0
dy = if length p1 > 2 && length p2 > 2 then p1 !! 2 - p2 !! 2 else 0
dz = if length p1 > 3 && length p2 > 3 then p1 !! 3 - p2 !! 3 else 0
c = 299792458.0
in -(c * dt) * (c * dt) + dx*dx + dy*dy + dz*dz
-- | Classify interval
intervalType :: Double -> String
intervalType s
| s < -1e-10 = "timelike" -- Can be connected by massive particle
| abs s < 1e-10 = "lightlike" -- Light cone / null
| otherwise = "spacelike" -- Causally disconnected
-- βββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββ
-- Light Cones
-- βββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββ
-- | Future light cone boundary (null surface)
-- (cΞt)Β² = ΞxΒ² + ΞyΒ² + ΞzΒ²
futureLightConeBoundary :: Vector -> Double -> Double -> [Vector]
futureLightConeBoundary (Vector center) radius c =
let angles = [0, pi/6 .. 2*pi]
conePoints = [ Vector [t, radius * cos a, radius * sin a, 0]
| t <- [0, 0.1 .. 1]
, a <- angles
]
in conePoints
-- βββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββ
-- Gravitational Time Dilation (General Relativity)
-- βββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββ
-- | Create Schwarzschild metric field (around non-rotating black hole)
schwarzschildField :: Double -> Double -> RelativityField
schwarzschildField mass_kg rs = RelativityField
{ relativityFieldId = "schwarzschild-" ++ show mass_kg
, relativityTimeDilation = \(Vector pos) ->
let r = if length pos >= 3
then sqrt (pos!!0*pos!!0 + pos!!1*pos!!1 + pos!!2*pos!!2)
else 1e6
in schwarzschildTimeDilation rs r 299792458.0
, localSpeedOfLight = 299792458.0
, gravitationalTimeWarp = \potential ->
sqrt (max 0.0001 (1.0 + 2.0 * potential / (299792458.0 ^ 2)))
, schwarzschildRadius = rs
}
-- | Create weak-field (post-Newtonian) relativity field
weakFieldRelativity :: Double -> RelativityField
weakFieldRelativity phi0 = RelativityField
{ relativityFieldId = "weak-field"
, relativityTimeDilation = \(Vector pos) ->
let r = if length pos >= 3
then sqrt (pos!!0*pos!!0 + pos!!1*pos!!1 + pos!!2*pos!!2)
else 1e6
phi = phi0 / r -- Newtonian potential β 1/r
in 1.0 + phi / (299792458.0 ^ 2) -- Post-Newtonian: g_tt β -(1 + 2Ο/cΒ²)
, localSpeedOfLight = 299792458.0
, gravitationalTimeWarp = \pot -> 1.0 + pot / (299792458.0 ^ 2)
, schwarzschildRadius = 0.0
}
-- βββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββ
-- Redshift / Blueshift
-- βββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββ
-- | Gravitational redshift (Doppler-like due to time dilation)
-- Ξ½_observer = Ξ½_source * β(g_tt_observer / g_tt_source)
gravitationalRedshift :: RelativityField -> Vector -> Vector -> Double -> Double
gravitationalRedshift field posSource posObs freq =
let dilationSource = relativityTimeDilation field posSource
dilationObs = relativityTimeDilation field posObs
in freq * sqrt (dilationObs / max 0.01 dilationSource)
-- βββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββ
-- WORM-sealed relativity observations
-- βββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββ
data RelativityObservation = RelativityObservation
{ relStep :: Int
, relPosition :: Vector
, relProperTime :: Double
, relTimeDilation :: Double
, relWormSeal :: String
} deriving (Show, Generic)
-- | WORM seal observation
sealRelativityObservation :: Int -> Vector -> RelativityField -> RelativityObservation
sealRelativityObservation step pos field =
let dilation = relativityTimeDilation field pos
properTime = localProperTime field pos 0.0 1.0 -- Unit global time
seal = "WORM[relativity:step=" ++ show step
++ ":pos=" ++ vectorToString pos
++ ":time_dilation=" ++ show (round (dilation * 10000) :: Integer)
++ "]"
in RelativityObservation step pos properTime dilation seal
-- | Vector to string for sealing
vectorToString :: Vector -> String
vectorToString (Vector xs) = "[" ++ unwords (map (\x -> take 6 (show x)) xs) ++ "]"
-- βββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββ
-- Special Relativity Configuration
-- βββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββββ
-- | Create special relativity field (flat spacetime)
specialRelativity :: RelativityField
specialRelativity = RelativityField
{ relativityFieldId = "special-relativity"
, relativityTimeDilation = \_ -> 1.0 -- No gravity
, localSpeedOfLight = 299792458.0
, gravitationalTimeWarp = \_ -> 1.0
, schwarzschildRadius = 0.0
}
-- | Create near-Schwarzschild field (e.g., around Sun)
sunField :: RelativityField
sunField =
let m_sun = 1.989e30 -- kg
g = 6.674e-11
c = 299792458.0
rs = 2.0 * g * m_sun / (c * c)
in schwarzschildField m_sun rs
|