Stopping Power for Light and Heavier Ions

Graphs, Data, Comments and Programs

This page will never be finished, but I keep trying!
Last update: 16 Oct 2015 (see bottom of page)

My name is Helmut Paul (b. 1929). Since 1990, I have been collecting data on stopping powers for light ions, while my colleagues at the University of Linz measured them. I plotted the data versus energy/nucleon, compared them to each other and to the theoretical or semi-empirical curves available in the literature. Together with A. Schinner, I produced a program MSTAR that will predict stopping powers for ions from 3Li to 18Ar (most recent version 3.12 of 2004). Our program JUDGE is used to compare stopping tables and experimental data in a statistical manner (see, e.g., papers below).

In recent years, the collection has been enlarged to include also all ions. It treats the electronic stopping power (we assume that “nuclear” stopping has been subtracted, but that need not always be true). It considers ordinary cold matter, not the plasma state. It considers gases and amorphous or polycrystalline solids.
Graphs are only shown where at least two or three data files are available for the particular ion and target, but all available experimental data are given in the data collection.
You are welcome to look at the plots, to use the data collection and to use program MSTAR. Although my collection is large, it is probably not complete. I keep it up to date, hoping that another expert (who??) will take over before I have to give up.

Since 2009, tables of Optical Oscillator Strengths have been listed for several elements, see below.

For recent discussions of stopping power data and of some related tables and programs, see papers by H. Paul and co-authors:
"An empirical approach to the stopping power of solids and gases for ions from Li to Ar",
              Nucl. Instr. Methods Phys. Res. B 179 (2001) 299,
"An empirical approach to the stopping power of solids and gases for ions from Li to Ar, Part II",
              Nucl.
Instr. Methods Phys. Res. B 195 (2002) 166,
"Judging the reliability of stopping power tables and programs for heavy ions",
              Nucl.
Instr. Methods Phys. Res. B 209 (2003) 252,
"Empirical stopping power tables for ions from 3Li to 18Ar and from 0.001 to 1000 MeV/nucleon in solids and gases",
              Atomic Data and Nuclear Data Tables 85 (2003) 377.

"Judging the reliability of stopping power tables and programs for protons and alpha particles using statistical methods",
              Nucl. Instrum. Methods. Phys. Res. B 227 (2005) 461
R.Bimbot, H.Geissel, H.Paul, A.Schinner, and P. Sigmund:
“ICRU Report 73: Stopping of Ions Heavier Than Helium”;
              J. of the ICRU 5, No.1 (2005)
“A comparison of recent stopping power tables for light and medium-heavy ions with experimental data, and applications to radiotherapy dosimetry",
              Nucl. Instrum. Methods Phys. Res. B 247 (2006) 166
"Statistical analysis of stopping data for protons and alphas in compounds",
              Nucl.
Instrum. Methods Phys. Res. B 249 (2006) 1
"New developments in stopping power for fast ions",
              Nucl.
Instrum. Methods Phys. Res. B 261 (2007) 1176
"Some new results on stopping power for fast ions",
              A.I.P. Conf. Proceedings 1099 (2009) 251
P.Sigmund, A.Schinner and H.Paul: "Errata and Addenda for ICRU Report 73, Stopping of Ions Heavier than Helium",
              J. of the ICRU (Oct. 8, 2009)
"Recent results in stopping power for positive ions, and some critical comments",
              Nucl. Instrum. Methods Phys. Res. B 268 (2010) 3421

H. Paul, “The stopping Power of Matter for Positive Ions”. In: Modern Practices in Radiation Therapy, ch. 7, G.Natanasabapathi (Ed.), InTech, ISBN 978-953-51-0427-8 (2012), available from http ://www.intechopen.com/books/modern-practices-in-radiation-therapy

Helmut Paul, "New results about stopping power for positive ions: Experiment and theory,
AIP Conf. Proc. 1525 (2013) 295

Helmut Paul and Daniel Sánchez-Parcerisa: “Acritical overview of recent stopping power programs for positive ions in solid elements
Nucl. Instr. Methods in Phys. Res. B 312 (2013) 110

Particular aspects of stopping power are discussed in the following papers:
Helmut Paul:
”A note on the Density Effect in the Stopping Power for positive Ions",
             Nucl. Instr. Methods Phys. Res. B 217 (2004) 7
H.Paul and A.Schinner:
"Does the Result of a Stopping Power Measurement Depend on the Method Used?",
             Physica Scripta 69 (2004) C41
Helmut Paul:
"On the Gas-Solid Difference in Stopping Power for low Energy Ions",
             Nucl. Instr. Methods Phys. Res. B 262 (2007) 13
Helmut Paul:
"Erratum to 'On the Gas-Solid Difference in Stopping Power for low Energy Ions'",
             Nucl. Instr. Methods Phys. Res. B 266 (2008) 857
Helmut Paul:
"The Solid-Gas Difference in Stopping Powers, and Statistical Analysis of Stopping Power Data",
             Nucl. Instr. and Meth. in Phys. Res. B 267 (2009) 9
H.Paul, P.L.Grande, D.Y.Smith:
"Optical Oscillator Strengths, Mean Excitation Energy, Shell Corrections and experimental values for Stopping Power",
              Nucl. Instr. and Meth. in Phys. Res. B 267 (2009) 2471
Helmut Paul: “Nuclear stopping power and its impact on the determination of electronic stopping power”,
             AIP Conf. Proc. 1525 (2013) 309
Helmut Paul and Daniel Sánchez-Parcerisa: “Acritical overview of recent stopping power programs for positive ions in solid elements
             Nucl. Instr. Methods in Phys. Res. B 312 (2013) 110

Applications to radiation therapy are discussed in the papers:
H.Paul, O.Geithner,O.Jaekel:
"The ratio of stopping powers of water and air for dosimetry applications in tumor therapy"
             Nucl. Instrum. Methods Phys. Res. B 256 (2007) 561
H.Paul, O.Geithner,O.Jaekel:
"The Influence of Stopping Powers upon Dosimetry for Radiation Therapy with Energetic Ions"
             Adv. Quantum Chem. 52 (2007) 289
H.Paul: "
The mean ionization potential of water,and its connection to the range of energetic carbon ions in water",
             Nucl. Instrum. Methods Phys. Res. B 255 (2007) 435
H.Paul: "
On the I values for Liquid Water used in ICRU Reports 49 and 73",
             ICRU News 2007 #1
H.Paul: “On the Accuracy of Stopping Power Codes and Ion Ranges used for Hadron Therapy”, pp. 39-61 in
            “Theory of Heavy Ion Collision Physics in Hadron Therapy”, D. Belkic, ed., Elsevier/Academic Press (2013), ISBN 978-0-12-396455-7

Introduction to Graphs and Data

Hydrogen Ions.

Earlier graphical presentations can be found in AZ77, Z77, ICRU49 and BP95 (these reference codes are explained in the list of stopping power tables and programs ).

See also: H. Paul, D. Semrad and A. Seilinger, "Reference stopping cross sections for hydrogen and helium ions in selected elements", Nucl. Instr. Methods in Phys. Res. B61 (1991) 261

Do you want to see the list of all the data for hydrogen ions available in my files? In this list, every line corresponds to one data file. The targets are ordered alphabetically. The headings in the list have the following meaning:

M

Mass Number of Projectile

Eq. Energy

Equivalent Proton Energy, i.e., energy of a proton of equal speed

Error

Error in percent. "e" means estimate.

Ref.

Reference Code, see list of all data references

Meas.

Number of measurement within the publication (you don’t need that!)

Method

Method of measurement according to classification by Paul, Semrad and Seilinger, Table 5

Ag.

State of aggregation (s: solid; g: gaseous). G: graphite (as opposed to amorphous carbon)

File

File designation: the file name Al.005, e.g., means file number 5 for hydrogen ions on Al.

In the graphs below, electronic stopping power in 10-15eV cm2/atom is plotted versus equivalent proton energy. Symbol A means file number 1 (e.g., file Al.001 for Al targets), symbol B means file number 2, etc. The data reference codes are explained in the list of all data references , and the curve designations in the list of stopping power tables and programs .

Graphs are only shown where at least two or three data files are available for the particular target. At present, graphs are available for the following targets:

Ions

Target

To see graph

Remark

H ions

Acetylene

Click here

 

H ions

Ag

Click here

At low energy, stopping is proportional to v, but at 1 keV, the proportionality constant changes (see Gö13)

H ions

Air

Click here

 

H ions

Al, versus v

Click here

For H in Al, stopping is proportional to velocity

H ions

Al

Click here

The new CasP version 3.0 is now correct down to 20 keV

H ions

Al2O3

Click here

The large binding effect of this compound is not well described by Ziegler’s program

H ions

Ar

Click here

Z03 agrees well with the data, ZBL85=Z92 was too low. After including electron capture, SG11 agrees with data at the maximum.

H ions

Au

Click here

A threshold for emission of 5d electrons has been found by Mk08 at 0.9 keV/nucleon.

H ions

Au, versus v

Click here

The measurements by Mk07 and Mk08 (similar to those by Fg07 for channeled ions) show a threshold effect at v = 0.19 v0. The theory byZeb12 shows a change of steepness there.

H ions

B

Click here

 

H ions

Be

Click here

 

H ions

Bi

Click here

Good agreement of Z03 with the data

H ions

Br

Click here

Excellent agreement between Ba84 and the Z03 curve for gaseous Br

H ions

C amorphous

Click here

The program by Grande and Schiwietz (GS00) using a single value for the mean excitation energy is low at the maximum, but agrees well with the data if different excitation energies are used for the subshells (GS00osc). The Op75 data appear high

H ions

Ca

Click here

At low energy, the Ep94a data are higher than all the semiempirical curves

H ions

Cd

Click here

Excellent agreement of Z03 with the scant data

H ions

Ce

Click here

The low Si72 data are apparently incorrect (see Kn80)

H ions

CH4

Click here

 

H ions

Cl

Click here

Excellent agreement between Z03 and the only data (Ba84)

H ions

Co

Click here

 

H ions

CO2

Click here

 

H ions

Cr

Click here

Good agreement of Z03 with all the data

H ions

Cu

Click here

The Gt62 and No75 data appear too low

H ions

Diamond

Click here

 

H ions

Ethylene

Click here

 

H ions

Fe

Click here

Good agreement of Z03 with all the data (except for Ar69)

H ions

Formvar

Click here

 

H ions

GaAs

Click here

 

H ions

GaSb

Click here

 

H ions

Gd

Click here

Excellent agreement of Z03 with the data, ICRU49 is too high

H ions

Ge, versus v

Click here

There is a clear threshold velocity

H ions

Ge

Click here

Discrepancy especially between Me82a and Ep92. But Mertens data before 1986 tend to be generally high

H ions

Graphite

Click here

 

H ions

H2

Click here

Z85 and Z89 are much too low here, but Z03 is good. The Cr42 data are too low

H ions

H2O Phase effect

Click here

The ICRU curves agree with the vapor data and with the Wenzel ice data within 2-3%. The gas-solid difference of ICRU ( 13%) is close to the experimental value.

H ions

H2O vapor

Click here

 

H ions

H2O cond. logar.

Click here

First measurements of stopping power of liquid water for protons!

H ions

H2O cond. linear

Click here

 

H ions

H2O liq. rel.

Click here

Relative graph shows discrepancies

H ions

Havar

Click here

Excellent agreement of the data with each other and with Z03

H ions

He

Click here

The two measurements Gl91 and RG01, though in mutual conflict, show a very strong threshold effect. At low energy, ICRU49 = AZ77 is too high (velocity proportional!). The theories GS93, Kim93 and Oliv94 support the Gl91 data, but not RG01. The Cab00 theory appears to support RG01, but it is too low since it considers only protons, not H atoms.

H ions

HfO2

Click here

 

H ions

Hydroxy apatite

Click here

 

H ions

In

Click here

Excellent agreement of Z03 with the data

H ions

Kapton (Polyimide)

Click here

 

H ions

KCl, versus v

Click here

The new Mk09 data show an extrapolated threshold

H ions

Kr

Click here

SG11 agrees with data at the maximum, due to inclusion of electron capture

H ions

Li

Click here

Z03 is good, but earlier versions are too low

H ions

LiF

Click here

 

H ions

LiF, versus v

Click here

The new Mk09 data show a stopping power threshold at v = 0.1 a.u. (250 eV/u)

H ions

LR-115

Click here

Cellulose Nitrate Nuclear Track Detector

H ions

Methane

Click here

 

H ions

Mg

Click here

The large gas-solid difference found by Bauer et al is not described by Ziegler’s program Z03

H ions

Mo

Click here

 

H ions

Mylar

Click here

 

H ions

N2

Click here

The low points due to B82a are for solid N2

H ions

Nb

Click here

The Bh73 data appear too low compared to Si84, Bi86, and Z03 is too high

H ions

Ne

Click here

CasP5.0 is too low, but SG11 agrees with data at the maximum, due to inclusion of electron capture

H ions

Ni

Click here

Here, there is an old discrepancy: many data are higher than the Linz data due to Se86a. It could be that many transmission measurements are high (cf. Mertens, Bauer, Semrad, Nucl. Instr. Meth. B15(1986) 91)

H ions

O2

Click here

Excellent agreement between all data and Z03

H ions

Pb

Click here

At low energy, the Ep92 data look unusual, but the Mont09a curve is close to them.

H ions

Pd

Click here

Excellent agreement of Z03 with the scant data

H ions

Polycarbonate

Click here

 

H ions

Polyethylene

Click here

 

H ions

Polypropylene

Click here

 

H ions

Polystyrene

Click here

 

H ions

Polyvinyltoluene

Click here

 

H ions

Propylene

Click here

 

H ions

Pt

Click here

Excellent agreement of Z03 with the data; ICRU49 is too high. At low energy, stopping is proportional to velocity (Gö13)

H ions

Rb

Click here

Z03 agrees very well with Ep94b; earlier curves are too low

H ions

Sb

Click here

Excellent agreement of Z03 with the data

H ions

Si

Click here

The Ar69 and Gm76 data appear too low. SRIM 2006 and SRIM 2003 give identical stopping powers

H ions

SiC

Click here

 

H ions

SiO2

Click here

 

H ions

SiO2, versus v

Click here

The Mk09a data show a threshold at low velocity

H ions

Sn

Click here

 

H ions

Sr

Click here

 

H ions

SrTiO3

Click here

 

H ions

Ta

Click here

The Si72 data appear too low compared to Lu79, Si84, etc.

H ions

Ti

Click here

The Gt62 and Ar69 data appear too high compared to Or71

H ions

V

Click here

Excellent agreement of Z03 with the data

H ions

W

Click here

Excellent agreement of Z03 with the data

H ions

Xe

Click here

Excellent agreement of Z03 with the data; ICRU 49 fits less well at 2000 keV

H ions

Y

Click here

At the maximum, all the curves are below the data

H ions

Yb

Click here

The low Si72 data are apparently incorrect (see Kn80)

H ions

Zn

Click here

The large gas-solid difference found by Bauer et al is not described by Ziegler’s program

H ions

ZnSiP2

Click here

 

H ions

Zr

Click here

Excellent agreement between Z03 and the scant data

To use the Origin files, click here to get file H-Files.zip which contains the compressed version of all the *.org files for H ions, and continue as outlined in Ch. 1.

Helium Ions.

Earlier graphical presentations can be found in Z77, ICRU49 and BP95 (these reference codes are explained in the list of stopping power tables and programs ).

See also: H. Paul, D. Semrad and A. Seilinger, "Reference stopping cross sections for hydrogen and helium ions in selected elements", Nucl. Instr. Methods in Phys. Res. B61 (1991) 261

Do you want to see the list of all the data for helium ions available in my files? The list was brought up to date in 2007. The headings are similar to those of the list for hydrogen ions (see above). In the graphs below, electronic stopping power in E(-15)eVcm2/atom is plotted versus equivalent alpha energy. Symbol A means file number 1 (e.g., file C.01 for C targets), symbol B means file number 2, etc. The data reference codes are explained in the list of all data references , and the curve designations in the list of stopping power tables and programs

Graphs are only shown where at least two or three data files are available for the particular target. At present, graphs are available for the following targets:

Ions

Target

To see graph

Remark

He Ions

Acetylene

Click here

 

He Ions

Ag

Click here

At low energy, stopping is proportional to velocity, but at 3 keV, the velocity constant changes (see Gö13)

He Ions

Air

Click here

 

He Ions

Al, versus v

Click here

For He in Al, stopping is velocity-proportional, but with different slopes in two different regions, indicating charge exchange between He and Al atoms

He Ions

Al

Click here

The first-principles charge-state calculation by Arnau et al. follows the data well except at the maximum. The new Bichsel calculation is slightly high at low energy

He Ions

Al2O3

Click here

 

He Ions

Ar

Click here

In agreement with Chu’s and Besenbacher’s measurements, Z03 (SRIM2003) predicts no gas-solid difference. Excellent agreement of Z03 and ICRU 49 with the data

He Ions

Au

Click here

Pe81 data are too high compared to many others

He Ions

Au, versus v

Click here

There is an indication of a stopping threshold similar to the case of H ions in Au. The theory by Zeb12 shows a change of steepness there.

He Ions

B

Click here

 

He Ions

Be

Click here

 

He Ions

Bi

Click here

Good agreement of Z03 with the data

He Ions

Butane

Click here

 

He Ions

C

Click here

Pe81 data are too high compared to many others

He Ions

Ca

Click here

Large discrepancy between Eppacher measurement and Z03

He Ions

CF4

Click here

 

He Ions

CO2

Click here

 

He Ions

CCl4 liquid, vapor

Click here

 

He Ions

Co

Click here

Excellent agreement of Z03 with the data

He Ions

Cr

Click here
Click here

The second graph shows the low energy data by Sp98 better; reevaluated Sp98 data are shown by circles (cf. remarks for Mo)

He Ions

Cu

Click here
Click here

The second graph shows the low energy data by Sp98 better; reevaluated Sp98 data are shown by circles (cf. remarks for Mo)

He Ions

Cyclohexane liquid, vapor

Click here

 

He Ions

Cyclopropane

Click here

 

He Ions

Dy

Click here

Good agreement of Z03 with most of the data

He Ions

Ethane

Click here

 

He Ions

Ethyl alcohol liquid

Click here

 

He Ions

Ethyl alcohol liquid, vapor

Click here

 

He Ions

Ethylene

Click here

 

He Ions

Fe

Click here

Good agreement of the curves (except for Z99) with most of the data

He Ions

Formvar

Click here

 

He Ions

GaSb

Click here

 

He Ions

Ge

Click here

 

He Ions

H2

Click here

Good agreement between Z03, ICRU 49 and the data

He Ions

H2S

Click here

 

He Ions

Havar

Click here

 

He Ions

He

Click here

Excellent agreement between curves and data (except for Hb72)

He Ions

Heptane liquid, vapor

Click here

 

He Ions

Hexane liquid, vapor

Click here

 

He Ions

HfO2

Click here

 

He ions

Hydroxy apatite

Click here

 

He Ions

InN

Click here

 

He Ions

Kapton, Polyimide

Click here

 

He Ions

KCl, versus v

Click here

The new Mk09 data show an (extrapolated) threshold

He Ions

Kr

Click here

Good agreement of Z03 and ICRU 49 with the data

He Ions

LiF, versus v

Click here

The new Mk09 data show a threshold at v = 0.1 a.u. (250 eV/u)

He Ions

Methane

Click here

 

He Ions

Methyl alcohol liquid, vapor

Click here

 

He Ions

Mg

Click here

 

He Ions

Mo

Click here
Click here

The Sp98 data are exceptional in that they go down as far as 0.01 keV (see the second graph). But these values are based on an evaluation of measured ranges for 5 - 100 keV He ions, taking the energy dependence from TRIM 95. We re-evaluated the Sp98 data by a comparison with Monte Carlo ranges from SRIM 2003 (circles).

He Ions

Mylar

Click here

 

He Ions

N2

Click here

Excellent agreement between curves and the data

He Ions

Ne

Click here

Excellent agreement between curves and data

He Ions

Ni

Click here
Click here

Excellent agreement of Z03 with the data above 20 keV. See also remark for Mo.

He Ions

O2

Click here

Excellent agreement between Z03, ICRU 49 and data

He Ions

Pb

Click here

 

He Ions

Pentane liquid, vapor

Click here

 

He Ions

3-Pentanone vapor

Click here

 

He Ions

Polycarbonate

Click here

 

He Ions

Polypropylene

Click here

 

He Ions

Polystyrene

Click here

 

He Ions

Polysulfone

Click here

 

He Ions

Propane

Click here

 

He Ions

Propyl alcohol vapor

Click here

 

He Ions

Propylene

Click here

 

He Ions

Propylene oxide vapor

Click here

 

He Ions

Pt

Click here

Good agreement between Z03 and the data. At low energy, stopping is proportional to velocity, but the velocity constant changes at 4 keV (Gö13).

He Ions

Se

Click here

Fair agreement of Z03 with the data, except for Co83

He Ions

SF6

Click here

 

He Ions

Si

Click here

The ICRU 49 curve appears slightly low at the maximum

He Ions

SiC

Click here

 

He Ions

SiO2

Click here

 

He Ions

SiO2, versus v

Click here

Contrary to the hydrogen data, the helium data do not show a threshold

He Ions

Sn

Click here

Good agreement of Z03 with the data except for Ep94a

He Ions

Ta

Click here

Excellent agreement of Z03 with the data

He Ions

Ta2O5

Click here

 

He Ions

Ti

Click here

Good agreement of the curves with the data (except for Gt62)

He Ions

V

Click here

Excellent agreement of Z03 with the data

He Ions

Vyns

Click here

 

He Ions

W

Click here

Good agreement

He Ions

Water

Click here

GarM09 curve reproduces the data quite well

He Ions

Water

Click here

 

He Ions

Water vapor

Click here

 

He Ions

Xe

Click here

Excellent agreement of Z03 with the data; ICRU 49 fits less well at 2000 keV

He Ions

Y

Click here

Fair agreement of Z03 with the data, except for Ep94a at low energy

He Ions

Zn

Click here

 

He Ions

ZnTe

Click here

 

He Ions

Zr

Click here

Good agreement of Z03 with the scant data

To use the Origin files, click here to get file He-Files.zip which contains the compressed version of all the *.org files for He ions, and continue as outlined in Ch. 1.

Heavier Ions

Do you want to see the List of all the data for heavier ions available in my files? See also the matrix which shows the number of available data files for all Z1 - Z2 - combinations, where Z1 is the atomic number of the projectile, Z2 that of the target. Z2 > 100 refers to mixtures and compounds. Please note that generally, graphs are only shown if at least three data files from different publications are available for the particular ion-target combination. So the data files are more complete than the graphs. In the graphs below, electronic stopping power in MeV/(mg/cm2) is plotted versus projectile energy per nucleon. Symbol A means file number 1, symbol B means file number 2, etc. The data reference codes are explained in the list of all data references , and the curve designations in the list of stopping power tables and programs . For ions up to Ti, there are also "universal plots" showing all the data obtained with one projectile. The data are divided by the electronic alpha stopping powers from ICRU Report 49, and normalized in such a way that they approach unity at high energy.

Graphs are only shown where at least two or three data files are available for the particular target. At present, graphs are available for the following projectiles and targets:

Projectiles

Target

To see graph:

Remarks

3Li ions

Ag

Click here

ICRU 73 is too high, CasP is too low at low energy

Air

Click here

Data by Hv71 appear low

Al

Click here

 

Ar

Click here

 

Au

Click here

Note that Ziegler's stopping power has been improved (increased) since Z92.

B

Click here

 

C

Click here

Here, many curves stay below the data at the maximum!

CH4

Click here

 

CO2

Click here

PASS too high at low energy

Cu

Click here

PASS too high

Gd

Click here

 

H2

Click here

 

He

Click here

Data by Hv71 appear low. PASS too high at low energy

Lu

Click here

 

Kapton

Click here

 

Mylar

Click here

 

N2

Click here

 

Ne

Click here

Data by Hv71 appear low. PASS too high at low energy

Ni

Click here

The BEST curve is only good at high energy. PASS too high

Pd

Click here

 

Polycarbonate

Click here

 

Polypropylene

Click here

 

Si

Click here

The measurements by BA09 (in bulk Si) are evidently too high at low energy. The CasP 4.0 curve is too low, while the ICRU73 curve is somewhat high

SiO2

Click here

 

Ta

Click here

 

Ti

Click here

 

Toluene

Click here

 

Water, liquid

Click here

 

Zn

Click here

 

Here is the universal plot for Li ions! To get the ORIGIN files, click here to get file Li-Files.zip, and continue as outlined in Ch. 1

4Be ions

Al

Click here

Point by Ang00 high compared to Zha02b

Au

Click here

 

C

Click here

 

Fe

Click here

 

He

Click here

 

Ne

Click here

 

Ni

Click here

 

Si

Click here

 

Zn

Click here

 

Here is the universal plot for Be ions! To get the ORIGIN files, click here to get file Be-Files.zip, and continue as outlined in Ch. 1

5B ions

Ag

Click here

 

Air

Click here

 

Al

Click here

 

Ar

Click here

 

Au

Click here

Data by Bt65 low compared to other data

B

Click here

 

C

Click here

 

Gd

Click here

 

Mylar

Click here

 

N2

Click here

 

Ni

Click here

Data by Bt65 low compared to other data

Poly carbonate

Click here

 

Si

Click here

This figure is quite similar to Fig. 14 of the Konac paper (KO98). Surprisingly, the Ziegler curve fits the data by the same group (Ds97) better than the Konac curve (KO98).

Zn

Click here

 

Here is the universal plot for B ions! To get the ORIGIN files, click here to get file B-Files.zip, and continue as outlined in Ch. 1

6C ions

Ag

Click here

 

Air

Click here

 

Al

Click here

 

Al2O3

Click here

 

Ar

Click here

The MSTAR curves follow the data points very well

Au

Click here

 

B

Click here

 

Be

Click here

Note the remarkable discrepancy between the (only) two data sets for C on Be!

C

Click here

The Ziegler, ATIMA, PASS and MSTAR curves fit the data quite well, the Konac curve (KO98) does not (at high energy because of the chosen I-value). Below the maximum, Geant4 becomes unreliable. CasP fits well except at low energy

Cu

Click here

 

Ge

Click here

 

Graphite

Click here

 

H

Click here

 

He

Click here

 

Kapton

Click here

 

Mylar

Click here

 

N

Click here

 

Ni

Click here

Hu00 Data appear too steep compared to Sa91, Po60, Ve79. In Hu00, the numbers in Table1 disagree with Fig. 1.

Polycarbonate

Click here

 

Polyvinyl chloride

Click here

 

Si

Click here

 

Silicon nitride

Click here

 

Silicon dioxide

Click here

 

Ta

Click here

 

Ti

Click here

 

Zr

Click here

 

ZrO2

Click here

 

Here is the universal plot for C ions! To get the ORIGIN files, click here to get file C-Files.zip, and continue as outlined in Ch. 1

7N ions

Ag

Click here

IDSA Data by Zi87 extrapolate to finite value for v=0: strange!
libdEdx, Jav12 and MNCPX are too low

Air

Click here

 

Al

Click here

Sa91 and Na68 data appear too high

Al2O3

Click here

 

Ar

Click here

Data by Fu96 very low compared to Or68, We53

Au

Click here

Nd77 data appear too steep

C

Click here

 

Cu

Click here

IDSA Data by Zi87 extrapolate to finite value for v=0: strange!

Ge

Click here

 

H

Click here

 

He

Click here

 

N

Click here

 

Kr

Click here

 

Mylar

Click here

 

Ne

Click here

 

Ni

Click here

IDSA Data by Zi87 extrapolate to finite value for v=0: strange!

Polycarbonate

Click here

 

Si

Click here

 

SiC

Click here

 

SiO2

Click here

 

Ta

Click here

 

Ti

Click here

 

Xe

Click here

 

Here is the universal plot for N ions! To get the ORIGIN files, click here to get file N-Files.zip, and continue as outlined in Ch. 1

8O ions

Ag

Click here

 

Air

Click here

 

Al

Click here

 

Al2O3

Click here

 

Ar

Click here

 

Au

Click here

Nd77 data appear too steep, see also 2001 paper by Paul and Schinner

B

Click here

 

Be

Click here

Note the remarkable discrepancy between the data sets Ch68 and Sa92, similar to the case of carbon ions on Be!

C

Click here

Below the maximum , Geant4 becomes unreliable, GS (CasP) is somewhat low. At the maximum, NS70 is slightly high

Cu

Click here

 

H2

Click here

 

He

Click here

The points at 95 MeV/nucleon appear high.

In

Click here

 

Kapton

Click here

 

Mylar

Click here

 

N2

Click here

 

Ne

Click here

 

Ni

Click here

 

O2

Click here

 

Poly carbonate

Click here

 

Si

Click here

 

SiC

Click here

 

Silicon nitride

Click here

 

Sn

Click here

 

Ta

Click here

 

Ta2O5

Click here

 

Ti

Click here

 

Zn

Click here

Combining the EFSR-TCS approach with CasP brings theory close to experiment

ZrO2

Click here

 

Here is the universal plot for O ions! To get the ORIGIN files, click here to get file O-Files.zip, and continue as outlined in Ch. 1

9F ions

Ag

Click here

 

Al

Click here

 

Au

Click here

 

C

Click here

 

Cu

Click here

 

Mo

Click here

 

N2

Click here

 

Ni

Click here

 

Poly- carbonate

Click here

 

Si

Click here

 

Ti

Click here

 

Here is the universal plot for F ions! To get the ORIGIN files, click here to get file F-Files.zip, and continue as outlined in Ch. 1

10Ne ions

Ag

Click here

Data by Tp62 low compared to other data

Air

Click here

 

Al

Click here

 

Ar

Click here

 

Au

Click here

The Nd77 data appear too steep (for other discrepant Nd77 data, see 2001 paper ).

C

Click here

The Po61 data appear high. Z98 lies high above Z96 and Z99.

H

Click here

 

He

Click here

At the maximum, the curves by Ziegler and MSTAR differ considerably, but there are no experimental points to decide.

N

Click here

 

Ni

Click here

 

Si

Click here

 

Here is the universal plot for Ne ions! To get the ORIGIN files, click here to get file Ne-Files.zip, and continue as outlined in Ch. 1

11Na ions

Air

Click here

 

Al

Click here

 

Ar

Click here

 

C

Click here

 

Mylar

Click here

 

Here is the universal plot for Na ions! To get the ORIGIN files, click here to get file Na-Files.zip, and continue as outlined in Ch. 1

12Mg ions

Ag

Click here

Note large discrepancy between data by At90 and Wr79, see also 2001 paper

Air

Click here

Data by Hv71 low compared to Fa68

Al

Click here

 

Au

Click here

Note large discrepancy between data by At90 and Wr79, see also 2001 paper

C

Click here

 

Cu

Click here

 

Fe

Click here

 

He

Click here

 

Ni

Click here

 

Poly- carbonate

Click here

 

Si

Click here

 

Ta

Click here

 

Here is the universal plot for Mg ions! To get the ORIGIN files, click here to get file Mg-Files.zip, and continue as outlined in Ch. 1

13Al ions

Ag

Click here

 

Al

Click here

 

Au

Click here

 

C

Click here

Data by Po61 low compared to Fa66. All the curves fit the data well

Mylar

Click here

Ziegler's (SRIM 2001) Bragg correction is visible: the corrected curve has a 5% step at 10 MeV (0.37 MeV/nucleon)

Ni

Click here

 

Poly- carbonate

Click here

 

SiC

Click here

 

Ta

Click here

 

Here is the universal plot for Al ions! To get the ORIGIN files, click here to get file Al-Files.zip, and continue as outlined in Ch. 1

14Si ions

Al

Click here

For comparison, "nuclear" stopping is shown as calculated by SRIM

Ag

Click here

 

Au

Click here

The Nd77 data appear low (for other discrepant Nd77 data, see 2001 paper ).

C

Click here

The KO98 curve is surprisingly high.

Cu

Click here

 

GaAs

Click here

 

Ge

Click here

 

Mylar

Click here

 

Ni

Click here

 

Polycarbonate

Click here

 

Polypropylene

Click here

 

Si

Click here

 

SiO2

Click here

Good agreement with ICRU73 and SRIM. MSTAR slightly low

W

Click here

 

Zr

Click here

 

Here is the universal plot for Si ions! To get the ORIGIN files, click here to get file Si-Files.zip, and continue as outlined in Ch. 1

15P ions

Al

Click here

 

C

Click here

 

Ge

Click here

 

Ni

Click here

 

Si

Click here

 

Here is the universal plot for P ions! To get the ORIGIN files, click here to get file P-Files.zip, and continue as outlined in Ch. 1

16S ions

Ag

Click here

 

Air

Click here

 

Ar

Click here

 

Au

Click here

Note that the (high) values of Bt66 are no more mentioned by Sd75, even though both publications have a common author . See 2001 paper by Paul and Schinner

C

Click here

 

Cu

Click here

 

H2

Click here

 

He

Click here

 

Kr

Click here

 

N2

Click here

 

Ni

Click here

 

Here is the universal plot for S ions! To get the ORIGIN files, click here to get file S-Files.zip, and continue as outlined in Ch.1

17Cl ions

Ag

Click here

 

Air

Click here

 

Al

Click here

 

Al2O3

Click here

 

Ar

Click here

 

Au

Click here

 

C

Click here

 

H2

Click here

 

He

Click here

 

Mylar

Click here

 

SiC

Click here

 

Silicon nitride

Click here

 

N2

Click here

 

Ni

Click here

 

Ta2O5

Click here

 

Here is the universal plot for Cl ions! To get the ORIGIN files, click here to get file Cl-Files.zip, and continue as outlined in Ch.1

18Ar ions

Ag

Click here

 

Air

Click here

 

Al

Click here

All the electronic stopping curves agree well with the data, except for Bar10 and libdEdx. "Nuclear" is the total nuclear stopping, integrated over all scattering angles, calculated using SRIM

Ar

Click here

 The Barbui curve (Barb10) fits the data well

Au

Click here

The Nd77 data are too low

Be

Click here

 

Butane

Click here

 

C

Click here

The low energy Trz02 data appear low. Jav12 fits well.

CH4

Click here

 

CO2

Click here

 

Cu

Click here

 

H2

Click here

Here, most of the curves (Ziegler, CasP, Hiraoka, Northcliffe) lie below the data, but MSTAR fits well

He

Click here

 

Kr

Click here

 

Mylar

Click here

 

N2

Click here

 

Ne

Click here

 

Ni

Click here

 

Poly carbonate

Click here

 

Si

Click here

 

Ta

Click here

 

Ti

Click here

 

Zr

Click here

 

Here is the universal plot for Ar ions! To get the ORIGIN files, click here to get file Ar-Files.zip, and continue as outlined in Ch.1

19K ions

C

Click here

 

Here is the universal plot for K ions! Click here to get file K-Files.zip which contains the compressed version of all the ORIGIN files for K ions, and continue as outlined in Ch.1

20Ca ions

C

Click here

 

Ni

Click here

 

Au

Click here

 

Here is the universal plot for Ca ions! Click here to get file Ca-Files.zip which contains the compressed version of all the *.org files for Ca ions, and continue as outlined in Ch.1

21Sc ions

C

Click here

 

Here is the universal plot for Sc ions! Click here to get file Sc-Files.zip which contains the compressed version of all the *.org files for Sc ions, and continue as outlined in Ch.1

22Ti ions

Ag

Click here

 

Al

Click here

 

Au

Click here

 

C

Click here

 

Cu

Click here

 

Ta

Click here

 

Here is the universal plot for Ti ions! Click here to get file Ti-Files.zip which contains the compressed version of all the ORIGIN files for Ti ions, and continue as outlined in Ch.1

24Cr ions

C

Click here

 

Click here to get file Cr-Files.zip which contains the compressed version of all the ORIGIN files for Cr ions

25Mn ions

C

Click here

 

Click here to get file Mn-Files.zip which contains the compressed version of all the ORIGIN files for Mn ions

26Fe ions

C

Click here

 

Click here to get file Fe-Files.zip which contains the compressed version of all the ORIGIN files for Fe ions

27Co ions

SiC

Click here

 

Click here to get file Co-Files.zip which contains the compressed version of all the ORIGIN files for Co ions

28Ni ions

Ag

Click here

Here, NS70 is low at the maximum

Al

Click here

The Hak02 data seem strange

C

Click here

 The theoretical program GB04 agrees beautifully with experiment at 1 MeV/nucleon

Cu

Click here

 

SiC

Click here

 

Click here to get file Ni-Files.zip which contains the compressed version of all the ORIGIN files for Ni ions

29Cu ions

Ag

Click here

 

Al

Click here

Here, NS70 is low at the maximum. Diwan01 extends the Hubert curve to lower energy. Jav12 fits the data

Au

Click here

 

C

Click here

Here, NS70 is low at the maximum

Cu

Click here

 

H2

Click here

 

SiC

Click here

 

Click here to get file Cu-Files.zip which contains the compressed version of all the ORIGIN files for Cu ions

32Ge ions

Ag

Click here

 

Al

Click here

 

C

Click here

 

Click here to get file Ge-Files.zip which contains the compressed version of all the ORIGIN files for Ge ions

33As ions

Si

Click here

 

Click here to get file As-Files.zip which contains the compressed version of all the ORIGIN files for As ions

35Br ions

Ag

Click here

 

Al

Click here

 

Au

Click here

 

C

Click here

 

Cu

Click here

 

SiC

Click here

 

Click here to get file Br-Files.zip which contains the compressed version of all the ORIGIN files for Br ions

36Kr ions

Ag

Click here

 

Al

Click here

The Northcliffe (NS) curve is low, while the Hubert curve (HU90) fits the data well

Ar

Click here

 

Au

Click here

 

Be

Click here

 

Butane

Click here

 

C

Click here

 Jav12 fits pretty well

Carbon dioxide

Click here

 

CF4

Click here

 

Cu

Click here

 

H2

Click here

 

He

Click here

 

Kr

Click here

 

Methane

Click here

 The Barbui curve (Barb10) fits the data very well

Mylar

Click here

 

N2

Click here

 

Ne

Click here

 

Ni

Click here

 

Si

Click here

 

Sn

Click here

 

Ta

Click here

 

Ti

Click here

 

Xe

Click here

 

Zr

Click here

 

Click here to get file Kr-Files.zip which contains the compressed version of all the ORIGIN files for Kr ions

41Nb ions

Ni

Click here

 

Ta

Click here

 

Click here to get file Nb-Files.zip which contains the compressed version of all the ORIGIN files for Nb ions

47Ag ions

Al

Click here

 

Fe

Click here

 

Ni

Click here

 

Pd

Click here

 

Ti

Click here

 

V

Click here

 

Zn

Click here

 

Zr

Click here

 

Click here to get file Ag-Files.zip which contains the compressed version of all the ORIGIN files for Ag ions

52Te ions

H2

Click here

 

Click here to get file Te-Files.zip which contains the compressed version of all the ORIGIN files for Te ions

53I ions

Ag

Click here

 

Al

Click here

The Barbui curve (Bar10) is too low at low energy

Au

Click here

 

C

Click here

 

Cu      

Click here

 

H2

Click here

 

Ni       

Click here

 

SiC

Click here

 

Click here to get file I-Files.zip which contains the compressed version of all the ORIGIN files for I ions

54Xe ions

Ag

Click here

 The Barbui curve (Bar10) is too low at low energy

Al

Click here

 The Barbui curve (Bar10) is too low at low energy; Jav12 fits pretty well

Ar

Click here

 

Au

Click here

 

Be

Click here

The point at 4 MeV/n is represented by Hubert, but not by Z03

C

Click here

Ziegler appears too low for light targets, but Hubert fits the data.

Cu

Click here

 

Ni

Click here

 

Pb

Click here

The Saxena results (nuclear track technique) appear strange

Si

Click here

 

Ti

Click here

 

Click here to get file Xe-Files.zip which contains the compressed version of all the ORIGIN files for Xe ions

74W ions

Au

Click here

 

Click here to get file W-Files.zip which contains the compressed version of all the ORIGIN files for W ions

79Au ions

Al

Click here

Click here

The ATIMA calculation reproduces the high energy data perfectly, while the Hubert and Ziegler tables are slightly low

Au

Click here

 Jav12 fits the data.

Butane

Click here

 

C

Click here

 

Cu

Click here

Click here

The ATIMA calculation reproduces the high energy data perfectly, while the Hubert and Ziegler tables are slightly low

Ni

Click here

 

Polystyrene

Click here

 

Si

Click here

 

SiC

Click here

 

Click here to get file Au-Files.zip which contains the compressed version of all the ORIGIN files for Au ions

82Pb ions

Al

Click here

 

Ar

Click here

 

Au

Click here

 

Be

Click here

The point at 4 MeV/n is represented by HU90, but not by Z03

C

Click here

Ziegler appears very low for light targets, but Hubert fits the data

Ni

Click here

 

Sn

Click here

 

Pb

Click here

 

Ti

Click here

 

Xe

Click here

 

Zr

Click here

 

Click here to get file Pb-Files.zip which contains the compressed version of all the ORIGIN files for Pb ions

83Bi ions

Ag

Click here

The Lindhard-Sörensen curve follows the high energy data better than SRIM (Z08)

Al

Click here

 

Au

Click here

 

Cu

Click here

The Lindhard-Sörensen curve follows the high energy data better than SRIM (Z08)

Pb

Click here

 

Ta

Click here

 

Click here to get file Bi-Files.zip which contains the compressed version of all the ORIGIN files for Bi ions

92U ions

Ag

Click here

 

Al

Click here

 

Ar

Click here

 The Barbui curve (Barb10) fits the data very well

Au

Click here

 SRIM is too high at the maximum for heavy ions in heavy targets, but Hubert fits the data

Be

Click here

 

Butane

Click here

 

C

Click here

SRIM is too low at the maximum for heavy ions in light targets, but Hubert fits the data

He

Click here

 

Kr

Click here

 

Mylar

Click here

 

N2

Click here

 

Ne

Click here

 

Ni

Click here

 

Ru

Click here

 

Ti

Click here

 

U

Click here

 

Xe

Click here

 

Zr

Click here

 

Click here to get file U-Files.zip which contains the compressed version of all the ORIGIN files for U ions

Computer Programs

In 2001, I have started to add links to computer programs : to our program MSTAR, and to those of other authors.

In the article "Empirical stopping power tables…” by H. Paul and A. Schinner published in Atomic Data and Nuclear Data Tables (see above), results of MSTAR are presented in tabular form.

Oscillations

If one plots the stopping power of one substance for various ions at constant, sufficiently low, velocity versus the atomic number of the ion, Z1, one obtains “Z1-oscillations” which correspond to the different atomic structures of the various ions. Similarly, graphs of the stopping power of one ion versus the atomic number of the target atom, Z2, show “Z2-oscillations”. Some examples are shown below.

Abscissa Z1

Target

 

Remark

Ag

Click here

 

Al

Click here

 

Au

Click here

 

C

Click here

 

Abscissa Z2

Ion

 

Remark

Cu

Click here

 

N

Click here

 

O

Click here

 

Please let me have your comments!
Helmut Paul
Institute for Experimental Physics
University of Linz
A-4040 Linz
Austria
Telephone: +43-732-2468-5333
Fax: +43-732-2468-8509

email: helmut.paul(/\t)jku.at

Back to beginning of Stopping Page?

Tables of Optical Oscillator Strengths. The optical oscillator strengths listed here for Al, Cu,and Au are due to J.M. Fernández-Varea, R. Mayol, D. Liljequist and F. Salvat, J. Phys.: Condens. Matter 5 (1993) 3593-3610. They are shown graphically in Fig. 1 of that paper.
The optical oscillator strengths for
Si are due to D.Y. Smith et al., see H. Paul, P.L.Grande, D.Y.Smith, "Optical Oscillator Strengths, Mean Excitation Energy, Shell Corrections and experimental values for Stopping Power" Nucl. Instrum. Methods B 267 (2009) 2471.

Last updates:

16 Oct 2015

Data for Nd, Pm, Sm in Cd, La in Sn, I in Ag, Cs in Sn (Pas15)

15 Apr 2015

Data for H and He ions in LiNbO3 (BA14b)

16 Mar 2015

Data for H and He ions in Zn and In (Gö14)

25 Oct 2014

Data for H and He ions in TiO2 (Lb96, Li14b); for H ions in H, He and N gas (Cn14)

12 Sep 2014

Theory for H in graphite, polystyrene (deVera14); for H, He, Li and Na in random graphene (Oja14). Data for C and Si ions in SiO2, and for C, Si and Cu ions in HfO2 (Msi14)

15 May 2014

Data for Li, C and O ions in Mylar, PEEK, polycarbonate (Mik14), for He in HfO2 (Pr14b); theory for H and He ions in LiF amd SiO2 (Mao 14)

26 Feb 2014

Data for Cl, Br, I, Au ions in SiC and SiO2 (Jin14); for U ions in Au (Ech13), Xe ions in C, Ni, Au (Ech14); H and He ions in hydroxyapatite (Li14); Au ions in SiC (Jin13); H ions in Pd (MS14); H ions in LiF (Dm13). Theory for H, He ions in Al, Au and H ions in LiF (Zeb12, Zeb13).

4 Feb 2014

Data for Mg, Al, Si in Formvar, Mg in Ta, Si in Ag, Al in Mylar (Gue14); for C, O, Cl, Br, I ions in Al2O3, Ta2O5, Si nitrate (Miz13); for Ne in Au (Pr13b) and H in HfO2 (Pr14). Theoretical curves for H in Si (Akk14), H in H2O (Sing14), H in water and methane (Mon14). Data for H in Ge (Rt13)

21 Jan 2014

Data for Ne in Au, for Kr in He, N2, Ne, Kr (Vok13).

16 Sep 2013

Data for U in C and Au, H in SrTiO3, Pd, Pt, Ag; He in Pt, Ag

25 Feb 2013

Single points from TEC13 for Cu, I and Au in O2, Si, Hf; Ni and Au in Ni; Ni and Br in Al2O3 and Ta2O5. C and O in Ta2O5. C, N, O, Si, Cl ions in silicon nitride

5 Feb 2013

Diwan01 fit curve for Cu in Al; new data by Pr12 for H, He in Au, Pt; by Chk12 for O, F, Si in Mylar. New data for C in Si; Ni,Cu, I, Au in C; I in Al; He, C, O in GaN and TiO2; Cl in Ta2O5; H,C in Al2O3; H, He in Formvar; C in ZrO2

21 Sep 2012

Low energy data for H, He in Al. Theories: Zeb12 for low energy H, He in Au, for H in H2O by Francis11. Fits by Jav12 for XeAl, ArC, KrC

17 Feb 2012

Fitted curves by Barb10 added. New version of theory by Schiwietz-Grande (SG11). Mylar data by Amm11.

12 Oct 2011

New data for H in water, for low energy H and He in Au and Cu, for He in InN, and for C and O in Zn. Accurate point for He in Si.

29 Mar 2011

New data for H, He, Li, B, Al, Mg, F, O, Br, I ions in Ag, Al, Au, Be, C, Ni, Si, Formvar, PHB, TiO2, UF4, ZrO2 by Dm10, Hs10, MD10, Msi10, Sik10, Brd67a and Brd67b.

20 Sep 2010

New graphs for H in He, Cu, LiF and in condensed H2O, for Li in Si and in polypropylene; new data for H in fluorides and in halogenated hydrocarbon compounds, and for Li, C, O in polypropylene added

26 Feb 2010

New data for H, He, Be, B, O, F, Ar, Kr, Au, U ions by Bbi10, BF09, Can09, CL09, Emf09, ZW09

11 Jan 2010

Theoretical curves for heavy ions added: CasP 4.0 and Arista09

20 Oct 2009

Theoretical curves for H, He in liquid water, and for H in W, Au, Pb and Bi. Low energy stopping values for H, He in LiF, KCl, and SiO2. New data for Xe and Y ions, for He, Li and heavy ions in Si, and for Ti in Au added.

23 Jun 2009

New data for H ions in Au, Si and liquid water and for He in Si added

12 Jun 2009

Theoretical END curves for hydrogen ions by Cab00, Cab02, Cab05, Cab08 and tables of optical oscillator strengths added.

29 Jan 2009

Stopping curves from Dent08 and data for Kr and Xe in silicon added. New version of data collection SCSData.zip

6 Nov 2008

Data for H in water vapor, Cl and Si in polymers, Li in Zn, and Au in Ni added

4 Sep 2008

Data for heavy ions in polymers, and for protons in AlF3 added

16 Jun 2008

Curve from YC02 for He in Si added

4 Jun 2008

Points due to Vs00 for H in Pd and Au corrected

26 May 2008

File SCSData.zip reinstalled that had been removed by mistake.

25 Apr 2008

Data for U ions by Brn72 added.

8 Feb 2008

Threshold effect for H and He in Au. Li ion data by YuH08. I reduced the size of the source code by a factor two using wordcleaner by textism.

12 Oct 2007

New data for He in Si and SiC, and for Cu in Au.

13 July 2007

Better presentation of gas/solid difference for He ions in gases. Update of *.zip files.

14 May 2007

Data by Hs07, Sun07, YuH07, and Zad07 added (not all in graphs)

7 March 2007

Section "Statistical Analysis" reorganized and beginning of page improved. Curves from Abr07 added to figures. Download of MSTAR corrected.

10 Jan 2007

Data by Fer06, Kny06, MP07, WD06, Zha06c added (not all in graphs)

31 Aug 2006

Data by Al04, HA05ab, Dm06, Per06, MM06, Fet06 added

14 Mar 2006

Recent articles added

13 Dec 2005

New data for air, H2, H2O, LiF, SiC, polycarbonate, aluminum oxide and other targets included

17 Oct 2005

Included new section with all the experimental data files

1 Sep 2005

PASS curves added to many graphs

26 Aug 2005

New section "Statistical Analysis" added

23 Jun 2005

Many additional data and corresponding graphs added, especially for H and He ions in (new) compounds

30 May 2005

List of compound targets brought up to date

4 Apr 2005

List of compound targets (for H and He ions) added

28 Nov 2004, 7 Feb 2005

Many additional data and new graphs added, especially for H and He ions in air and compounds. Zip files brought up to date

1 Sep 2004

Some new graphs and remarks for H, He, and Li ions

24 Jun 2004

Many comments added to graphs for H and He ions

16 Jun 2004

Recent data added for various ions in Si, and for Au, Pb, and U projectiles

29 May 2004

Naglib routine S15AEF in MSTAR replaced by a local routine (MSTAR 3.12)

22 Apr 2004

Recent data added for He ions in Ag, Ar, Au, Cr, Cu, He, Kr, Mg, Mo, N2, Ne, Ni, O2, Ti, Xe. New graphs for H ions in Br, Cl, and Graphite.

26 Mar 2004

Data added for He ions in Al, Ar, Be, Bi, C, Co, Cr, Cu, Dy, Fe, Ge, H2, He, Kr, Mo, N2, Ne, Ni, O2, Pb, Se, Si, Sn, Ta, Ti, V, W, Xe,, Y. Many new graphs.

11 Mar 2004

Data added for H ions in Au, Be, C, Cd, Cr, Cu, H, He, In, N, Ni, Pb, Pd, Sn, Xe, Zr; for He ions in Ag, Au, Si; for Li ions in Cu, Zn; for N ions in Au. Corresponding zip-files updated

22 Dec 2003

Data added for Li ions.

New or updated graphs for H ions in H2, He, Be, N2, O2, Mg, Al, Ti, V, Fe, Co, Ni, Cu, Ge, Mo, Ag, Sn, Sb, Ta, Pt, Au, Pb, and Bi targets. New list of data files for H ions.

14 Nov 2003

New graphs added for H, Li, C, Mg, and Ag ions; zip files updated, Ag-Files.zip new.

9 Jul 2003

New graphs for Li, O, Ti, Nb, Xe, W, Au, Pb and U ions

26 Jun 2003

*.zip files containing ORIGIN files updated. New section ?Oscillations? added

28 May 2003

Graphs for H ions with gas-solid effect. Some data by Whl02 (in Si) added; also LiX02b

8 Apr 2003

New version 3.11 of MSTAR also calculates B, Zr, and Ta targets

3 Apr 2003

Graphs for new targets: B, Ta, Zr

1 Apr 2003

Many new targets for Kr ions added

13 Feb 2003

Many compounds added

06 Feb 2003

Several Z03 curves added. Universal plots renewed.

24 Jan 2003

*.zip files containing ORIGIN files updated

02 Dec 2002

New version (3.00) of MSTAR, based on the new data, and nickel target data

04 Sep 2002

Added new data by Ala01, Ala02, Ara02, Aze02, Hak02, Kha01, LiX02, Pen01, Shr02, Trz02, Whl02a, Zha02b. Redundant data by Hv68 removed.

12 Mar 2002

Mylar, Kapton and graphite graphs added. Also curves by Northcliffe and Geant4

21 Nov 2001

Structure of page reorganised. Data files up to 36Kr ions completed. Some graphs for Xe and U ions added.

17 Oct 2001

Some graphs corrected, Mylar data added, Hiraoka and MSTAR curves added, tables updated

15 Oct 2001

Links to computer programs added

19 Jul 2001

*.zip files updated, some new. Universal curves updated

27 Jun 2001

Data for K, Ar, Ca, Sc, Ti ions added

9 May 2001

An78 data (Li ions) added, Bi90 data (O ions) removed, LuX00 data (O and F ions) added

13 Nov 2000

Universal curves added; Li ions on Al, C ,Cu ,H2 ,He ,Ne ,Ni; B on Al, C; O on C, Ni

6 Sep 2000

C, N, O on carbon; O on aluminum

30 May 2000

New graphs for gas targets. New data by Hu99, Ang00, Hu00, She00 for solid targets

6 Apr 2000

Improved graphs for C, O, Ar projectiles (new Ziegler and GS curves), etc.

15 Mar 2000

New/improved graphs: H on Al, C, Gd, Pt, Ta, W; C on Ag, Au; S on Ag, H, Kr;Cl on Ar, H

10 Jan 2000

Additional points by Si84 for H on Al, Gd, Pt, Ta, and W

21 Dec 1999

New graphs: H on Gd,Pt; B on Ag,Au; Mg on Ag,Al. Others improved.

24 Nov 1999

Improved layout, and some new data.

18 Oct 1999

Correction: Points of Po60 for O projectiles had been plotted at wrong energies.