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Geant4/examples/advanced/underground_physics/README

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Differences between /examples/advanced/underground_physics/README (Version 11.3.0) and /examples/advanced/underground_physics/README (Version 11.2)


  1 ------------------------------Advanced Example      1 ------------------------------Advanced Example---------------------------------         README FILE
  2                                                     2 
  3 Note: Due to the importation of data files dur      3 Note: Due to the importation of data files during the initialisation stage of
  4 Geant4, load-time may be in excess of 5 minute      4 Geant4, load-time may be in excess of 5 minutes.
  5                                                     5 
  6 UNDERGROUND PHYSICS                                 6 UNDERGROUND PHYSICS
  7                                                     7 
  8 An example of a underground dark matter experi      8 An example of a underground dark matter experiment.
  9                                                     9 
 10 Please see the UserRequirements.txt and relate     10 Please see the UserRequirements.txt and related web-pages referred to
 11 at the end of that document.                       11 at the end of that document.
 12                                                    12 
 13 Over-view:                                         13 Over-view:
 14 A single liquid xenon cell is simulated within     14 A single liquid xenon cell is simulated within Geant4 and the scintillation
 15 light produced from interactions from various      15 light produced from interactions from various calibration species is recorded
 16 as PhotoMultiplier hits.  The output is then w     16 as PhotoMultiplier hits.  The output is then written to an ASCII file for
 17 future off-line analysis.                          17 future off-line analysis.
 18                                                    18 
 19 Geometry:                                          19 Geometry:
 20 Experimental set-up:                               20 Experimental set-up:
 21                                                    21 
 22   G4double worldWidth  = 470.0*cm + 2.*wallThi     22   G4double worldWidth  = 470.0*cm + 2.*wallThick; // "x"
 23   G4double worldLength = 690.0*cm + 2.*wallThi     23   G4double worldLength = 690.0*cm + 2.*wallThick; // "y"
 24   G4double worldHeight = 280.0*cm + 2.*wallThi     24   G4double worldHeight = 280.0*cm + 2.*wallThick; // "z"
 25                                                    25 
 26                                                    26 
 27                                                    27 
 28 A "cavern" of dimensions 5.18m x 7.38m x 3.28m     28 A "cavern" of dimensions 5.18m x 7.38m x 3.28m with concrete walls is defined
 29 as the World Volume.  A laboratory geometry is     29 as the World Volume.  A laboratory geometry is incorporated included desks,
 30 cupboards, door and windows.  For ease this is     30 cupboards, door and windows.  For ease this is included in a separate ".icc"
 31 file which can be removed should the code seem     31 file which can be removed should the code seem cumbersome.  In the centre of 
 32 the cavern a steel vacuum vessel containing li     32 the cavern a steel vacuum vessel containing liquid and gaseous xenon is placed.
 33 The internal construction of the vessel accura     33 The internal construction of the vessel accurately reproduces an existing 
 34 prototype Dark Matter detector which allows ex     34 prototype Dark Matter detector which allows experimental comparison. The active
 35 detector volume is defined by a series of meta     35 detector volume is defined by a series of metal rings, complemented by
 36 a cover mirror and a PMT immersed in the liqui     36 a cover mirror and a PMT immersed in the liquid.  Two grids and a
 37 thermalising copper shield are also incorporat     37 thermalising copper shield are also incorporated. The liquid/gas
 38 interface is located 6mm away from the mirror      38 interface is located 6mm away from the mirror surface. A Am241
 39 calibration source is suspended from one of th     39 calibration source is suspended from one of the grids in the liquid
 40 phase, above the PMT.                              40 phase, above the PMT.
 41                                                    41 
 42       XXX================XXX mirror                42       XXX================XXX mirror
 43       XXX________________XXX gas phase             43       XXX________________XXX gas phase
 44       XXX                XXX                       44       XXX                XXX 
 45       XXX                XXX liquid phase          45       XXX                XXX liquid phase
 46       XXX                XXX                       46       XXX                XXX
 47       XXX.......U........XXX grid + calibrator     47       XXX.......U........XXX grid + calibrator
 48       XXX................XXX grid                  48       XXX................XXX grid
 49       XXX|              |XXX                       49       XXX|              |XXX
 50          | ___------___ |                          50          | ___------___ | 
 51          ||    PMT     ||                          51          ||    PMT     ||
 52          ||            ||                          52          ||            ||
 53                                                    53 
 54                                                    54 
 55 Hits Output (file "hits.out"):                     55 Hits Output (file "hits.out"):
 56 An ASCII file containing the following informa     56 An ASCII file containing the following information:
 57      Evt #         : event number                  57      Evt #         : event number
 58      Etot, MeV     : energy deposited in liqui     58      Etot, MeV     : energy deposited in liquid xenon
 59      LXe hits      : number of hits in liquid      59      LXe hits      : number of hits in liquid xenon
 60      LXeTime, ns   : time of first hit in liqu     60      LXeTime, ns   : time of first hit in liquid xenon
 61      PMT hits      : number of hits in PMT (ph     61      PMT hits      : number of hits in PMT (photocathode)
 62      PmtTime, ns   : average PMT hit time rela     62      PmtTime, ns   : average PMT hit time relative to LXeTime
 63      First hit     : first particle to hit liq     63      First hit     : first particle to hit liquid xenon
 64      Flags         : particles contributing to     64      Flags         : particles contributing to energy deposition
 65      Seeds     : the initial seed values for g     65      Seeds     : the initial seed values for given hit events
 66                                                    66 
 67      Note:                                         67      Note:
 68                                                    68 
 69      The time information PmtTime is erroneous     69      The time information PmtTime is erroneous when forcing nuclear
 70      decay with the RadioactiveDecay module du     70      decay with the RadioactiveDecay module due to the precision
 71      required to detect nanosecond scintillati     71      required to detect nanosecond scintillation times on a global
 72      time of 432 years (in the case of 241Am d     72      time of 432 years (in the case of 241Am decay).
 73                                                    73 
 74                                                    74 
 75 Pmt Output (file "pmt.out"):                       75 Pmt Output (file "pmt.out"):
 76 Photon hit positions within the PMT face (over     76 Photon hit positions within the PMT face (overwritten every event):
 77 "Hit#    X, mm   Y, mm   Z, mm"                    77 "Hit#    X, mm   Y, mm   Z, mm"
 78                                                    78 
 79                                                    79 
 80 To Run:                                            80 To Run:
 81 Either run the macro files interactively or in     81 Either run the macro files interactively or in batch with the command
 82 DMX macro_name.mac.                                82 DMX macro_name.mac.
 83                                                    83 
 84                                                    84 
 85 Macros:                                            85 Macros:
 86                                                    86 
 87    initInter.mac                                   87    initInter.mac
 88    Initialisation macro for interactive mode.      88    Initialisation macro for interactive mode.
 89                                                    89 
 90    gamma.mac                                       90    gamma.mac
 91    Shoots one 60 keV gamma upwards from the ca     91    Shoots one 60 keV gamma upwards from the calibrator and traces the
 92    scintillation light produced in LXe to the      92    scintillation light produced in LXe to the PMT. All tracks are drawn
 93    with custom colours. PMT hits in photocatho     93    with custom colours. PMT hits in photocathode are also shown. Event
 94    summary is writen to file "hits.out".           94    summary is writen to file "hits.out".
 95                                                    95 
 96    gamma_1000.mac                                  96    gamma_1000.mac 
 97    Similar to above, but 1000 gammas are emmit     97    Similar to above, but 1000 gammas are emmited isotropically from the
 98    source. No hits or tracks are draw, and the     98    source. No hits or tracks are draw, and the verbosity is reduced.
 99                                                    99 
100    alpha.mac                                      100    alpha.mac
101    Shoots one 5.486 MeV alpha particle upwards    101    Shoots one 5.486 MeV alpha particle upwards from the calibrator and
102    traces the scintillation light to the PMT.     102    traces the scintillation light to the PMT. All tracks except
103    optical photons are drawn. Event summary is    103    optical photons are drawn. Event summary is written to file
104    "hits.out" and PMT hits to file "pmt.out".     104    "hits.out" and PMT hits to file "pmt.out".
105                                                   105 
106    alpha_1000.mac                                 106    alpha_1000.mac
107    Similar to above, but 1000 alphas are emmit    107    Similar to above, but 1000 alphas are emmited isotropically from the
108    source. No tracks are stored, and the verbo    108    source. No tracks are stored, and the verbosity is reduced. Event
109    summary is written to file "hits.out", PMT     109    summary is written to file "hits.out", PMT hits are not written out.
110                                                   110 
111    neutron.mac                                    111    neutron.mac
112    Shoots one 2.48 MeV neutron inside the room    112    Shoots one 2.48 MeV neutron inside the room aimed at the detector. 
113    All tracks except scintillation photons are    113    All tracks except scintillation photons are drawn (custom colours).
114    Gammas are not killed at the concrete wall.    114    Gammas are not killed at the concrete wall. Event summery is written
115    to file "hits.out".                            115    to file "hits.out".
116                                                   116 
117    ambe_spectrum.mac                              117    ambe_spectrum.mac
118    Produces a spectrum of neutrons according t    118    Produces a spectrum of neutrons according to an approximation of a Am/Be
119    neutron source.  However, this uses the GPS    119    neutron source.  However, this uses the GPS and therefore will only work
120    after compilation with the DMXENV_GPS_USE e    120    after compilation with the DMXENV_GPS_USE environment variable (see below)
121                                                   121 
122                                                   122 
123    sourceAm241.mac                                123    sourceAm241.mac
124    Forces the decay of 241Am nuclei in the cal    124    Forces the decay of 241Am nuclei in the calibrator and tracks the
125    resulting particles (237Np + alpha + gamma     125    resulting particles (237Np + alpha + gamma from 237Np
126    de-excitation). All tracks are drawn except    126    de-excitation). All tracks are drawn except scintillation photons.
127    Event summery is written to file "hits.out"    127    Event summery is written to file "hits.out".   
128    -> To be added for a future release            128    -> To be added for a future release
129                                                   129 
130                                                   130 
131    sourceAm241_1000.mac                           131    sourceAm241_1000.mac
132    Similar to above but for 1000 events. No tr    132    Similar to above but for 1000 events. No tracks are stored.
133    -> To be added for a future release            133    -> To be added for a future release
134                                                   134 
135                                                   135 
136 Note:                                             136 Note: 
137 The following environment variables need to be    137 The following environment variables need to be set:
138 G4RADIOACTIVEDATA      : points to Radioactive    138 G4RADIOACTIVEDATA      : points to Radioactive Decay Data files
139 G4LEDATA               : points to low energy     139 G4LEDATA               : points to low energy data base
140 G4LEVELGAMMADATA       : points to PhotoEvapor    140 G4LEVELGAMMADATA       : points to PhotoEvaporation data
141 NeutronHPCrossSections : points to neutron dat    141 NeutronHPCrossSections : points to neutron data files
142                                                   142 
143 In addition if you require to use the full Gen    143 In addition if you require to use the full General Particle Source then the
144 variable DMXENV_GPS_USE can be set.  The DMX g    144 variable DMXENV_GPS_USE can be set.  The DMX gun is still included in order to
145 allow forward compatibility should the GPS cha    145 allow forward compatibility should the GPS change.
146                                                   146 
147                                                   147 
148 ANALYSIS:                                         148 ANALYSIS:
149                                                   149 
150 The program should produce ROOT-based histogra    150 The program should produce ROOT-based histogram files. It is possible to 
151 produce the output in XML-compliant format by     151 produce the output in XML-compliant format by changing the G4AnalysisManager default file type in DMXRunAction::Book().
152                                                   152 
153 SEEDS:                                            153 SEEDS:
154                                                   154 
155 The seeds of event hits are stored in the hit     155 The seeds of event hits are stored in the hit record file.  These can be used
156 to repeat events for visualisation, test crash    156 to repeat events for visualisation, test crashes/idiosyncracies:
157                                                   157 
158 /random/setDirectoryName ./seeds                  158 /random/setDirectoryName ./seeds
159 /random/resetEngineFrom currentEvent.rndm         159 /random/resetEngineFrom currentEvent.rndm
160 /random/saveThisEvent                             160 /random/saveThisEvent
161 /random/setSavingFlag                             161 /random/setSavingFlag
162                                                   162 
163 The file currentEvent.rndm should contain the     163 The file currentEvent.rndm should contain the two seeds which were outputed in
164 the scintHit file.                                164 the scintHit file.
165                                                   165 
166 ERRORS:                                           166 ERRORS:
167                                                   167 
168 When running interactively the following error    168 When running interactively the following error will be shown:
169                                                   169 
170 BooleanProcessor::caseIE : unimplemented case     170 BooleanProcessor::caseIE : unimplemented case
171 BooleanProcessor::caseIE : unimplemented case     171 BooleanProcessor::caseIE : unimplemented case
172 BooleanProcessor::caseIE : unimplemented case     172 BooleanProcessor::caseIE : unimplemented case
173 BooleanProcessor::caseIE : unimplemented case     173 BooleanProcessor::caseIE : unimplemented case
174 BooleanProcessor::caseIE : unimplemented case     174 BooleanProcessor::caseIE : unimplemented case
175 BooleanProcessor::caseIE : unimplemented case     175 BooleanProcessor::caseIE : unimplemented case
176 BooleanProcessor: boolean operation failed        176 BooleanProcessor: boolean operation failed
177 BooleanProcessor::caseIE : unimplemented case     177 BooleanProcessor::caseIE : unimplemented case
178 BooleanProcessor::caseIE : unimplemented case     178 BooleanProcessor::caseIE : unimplemented case
179 BooleanProcessor::caseIE : unimplemented case     179 BooleanProcessor::caseIE : unimplemented case
180 BooleanProcessor::caseIE : unimplemented case     180 BooleanProcessor::caseIE : unimplemented case
181 BooleanProcessor: boolean operation failed        181 BooleanProcessor: boolean operation failed
182                                                   182 
183 This is a "feature" of the visualisation of bo    183 This is a "feature" of the visualisation of boolean volumes, but does not
184 affect functionality/performance so can be ign    184 affect functionality/performance so can be ignored.
185                                                   185 
186 NB:                                               186 NB:
187 If using explicit libraries (?) i.e. non-share    187 If using explicit libraries (?) i.e. non-shared then compilation time with
188 neutrons in physics list is very long (>5 minu    188 neutrons in physics list is very long (>5 minutes) - check this.............
189 It is more efficient to use shared libraries t    189 It is more efficient to use shared libraries that are loaded at run-time with
190 increased initialisation time (at run-time).      190 increased initialisation time (at run-time).
191                                                   191 
192 Also if using shared libraries the load time a    192 Also if using shared libraries the load time at run-time may be several minutes
193 - this is partially due to the neutron impleme    193 - this is partially due to the neutron implementation requires full data sets
194 for each isotope being specified.                 194 for each isotope being specified.
195                                                   195 
196                                                   196 
197 --------------------------------------            197 --------------------------------------
198                                                   198 
199 If running on Redhat 7.0 or above set G4SYSTEM    199 If running on Redhat 7.0 or above set G4SYSTEM to Linux-g++, alternatively you
200 can install backward compatibility to egcs, ho    200 can install backward compatibility to egcs, however, requires
201 config/sys/Linux-egcs.gmk to be altered so tha    201 config/sys/Linux-egcs.gmk to be altered so that CXX is set to kgcc 
202 (compared to g++ in original file)                202 (compared to g++ in original file)
203                                                   203 
204 --------------------------------------            204 --------------------------------------
205                                                   205 
206                                                   206 
207 Alex Howard, 29/11/01                             207 Alex Howard, 29/11/01
208 updated 18/06/02                                  208 updated 18/06/02
209                                                   209