File: ackermann.ruby-5.ruby

package info (click to toggle)
jruby 9.4.8.0%2Bds-3
  • links: PTS, VCS
  • area: main
  • in suites: forky, sid, trixie
  • size: 89,244 kB
  • sloc: ruby: 548,574; java: 276,189; yacc: 25,873; ansic: 6,178; xml: 6,111; sh: 1,855; sed: 94; makefile: 78; jsp: 48; tcl: 40; exp: 12
file content (153 lines) | stat: -rw-r--r-- 3,151 bytes parent folder | download | duplicates (9)
1
2
3
4
5
6
7
8
9
10
11
12
13
14
15
16
17
18
19
20
21
22
23
24
25
26
27
28
29
30
31
32
33
34
35
36
37
38
39
40
41
42
43
44
45
46
47
48
49
50
51
52
53
54
55
56
57
58
59
60
61
62
63
64
65
66
67
68
69
70
71
72
73
74
75
76
77
78
79
80
81
82
83
84
85
86
87
88
89
90
91
92
93
94
95
96
97
98
99
100
101
102
103
104
105
106
107
108
109
110
111
112
113
114
115
116
117
118
119
120
121
122
123
124
125
126
127
128
129
130
131
132
133
134
135
136
137
138
139
140
141
142
143
144
145
146
147
148
149
150
151
152
153
#!/usr/bin/ruby
# The Computer Language Benchmark Shootout
# http://shootout.alioth.debian.org
#
# original code by Martin DeMello
# modified by Jabari Zakiya 3/20/05
# modified by Glenn Parker 3/28/05 (format results)

include Math

SOLAR_MASS = 4*PI*PI
DAYS_PER_YEAR = 365.24

Vector3D = Struct.new("Vector3D", :x, :y, :z)

class Vector3D

  def *(val)
    Vector3D.new(*self.map {|i| i * val})
  end

  def /(val)
    Vector3D.new(*self.map {|i| i / val})
  end

  #in-place add with scale
  # a.adds(b, s) -> a += b*s

  def adds(other, scale)
    self[0] += other[0]*scale; self[1] += other[1]*scale
    self[2] += other[2]*scale
  end

  def subs(other, scale)
    self[0] -= other[0]*scale; self[1] -= other[1]*scale
    self[2] -= other[2]*scale
  end

  def magnitude
    x=self[0]; y=self[1]; z=self[2]
    sqrt(x*x + y*y + z*z)
  end

  # |self - other|
  def dmag(other)
    x=self[0]-other[0]; y=self[1]-other[1]; z=self[2]-other[2]
    sqrt(x*x + y*y + z*z)
  end
end

class Planet
  attr_accessor :pos, :v, :mass

  def initialize(x, y, z, vx, vy, vz, mass)
    @pos = Vector3D.new(x, y, z)
    @v = Vector3D.new(vx, vy, vz) * DAYS_PER_YEAR
    @mass = mass * SOLAR_MASS
  end

  def distance(other)
    self.pos.dmag(other.pos)
  end
end

jupiter = Planet.new(
   4.84143144246472090e+00,
   -1.16032004402742839e+00,
   -1.03622044471123109e-01,
   1.66007664274403694e-03,
   7.69901118419740425e-03,
   -6.90460016972063023e-05,
   9.54791938424326609e-04)

saturn = Planet.new(
   8.34336671824457987e+00,
   4.12479856412430479e+00,
   -4.03523417114321381e-01,
   -2.76742510726862411e-03,
   4.99852801234917238e-03,
   2.30417297573763929e-05,
   2.85885980666130812e-04)

uranus = Planet.new(
   1.28943695621391310e+01,
   -1.51111514016986312e+01,
   -2.23307578892655734e-01,
   2.96460137564761618e-03,
   2.37847173959480950e-03,
   -2.96589568540237556e-05,
   4.36624404335156298e-05)

neptune = Planet.new(
   1.53796971148509165e+01,
   -2.59193146099879641e+01,
   1.79258772950371181e-01,
   2.68067772490389322e-03,
   1.62824170038242295e-03,
   -9.51592254519715870e-05,
   5.15138902046611451e-05)

sun = Planet.new(0, 0, 0, 0, 0, 0, 1)

class Array
  def each_pair
    a = []
    each_index {|i|
      ((i+1)...length).each {|j|
        yield at(i), at(j)
      }
    }
  end
end

bodies = [sun, jupiter, saturn, uranus, neptune]

class << bodies
  def advance(dt)
    mag = m1 = m2 = nil
    each_pair {|b1, b2|
      d = b1.distance(b2)
      mag = dt/(d*d*d)

      m1 = b1.mass * mag
      m2 = b2.mass * mag

      b1.v.adds(b2.pos, m2)
      b1.v.subs(b1.pos, m2)
      b2.v.adds(b1.pos, m1)
      b2.v.subs(b2.pos, m1)
    }

    each {|b| b.pos.adds(b.v, dt)}
  end

  def energy
    e = 0
    each {|b| e += 0.5 * b.mass * (b.v.magnitude ** 2) }
    each_pair {|b1, b2| e -= (b1.mass * b2.mass) / b1.distance(b2) }
    e
  end

  def offset_momentum
    p = Vector3D.new(0,0,0)
    sun = self[0]
    each {|b| p.adds(b.v, b.mass) }
    sun.v.subs(p, 1.0/sun.mass)
  end
end

bodies.offset_momentum
puts "%.9f" % bodies.energy
Integer(ARGV[0]).times { bodies.advance(0.01) }
puts "%.9f" % bodies.energy