https://github.com/pumpncode/latakama
https://github.com/pumpncode/latakama
Last synced: 4 months ago
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- Host: GitHub
- URL: https://github.com/pumpncode/latakama
- Owner: pumpncode
- License: 0bsd
- Created: 2025-03-01T13:06:10.000Z (over 1 year ago)
- Default Branch: main
- Last Pushed: 2025-04-07T01:44:49.000Z (about 1 year ago)
- Last Synced: 2025-09-11T00:37:04.765Z (9 months ago)
- Language: Mathematica
- Size: 198 KB
- Stars: 0
- Watchers: 1
- Forks: 0
- Open Issues: 0
-
Metadata Files:
- Readme: readme.md
- License: license.md
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README
# latakama
The latakama is a system of units of measurement based on universal physical constants and dimensionless quantities. The planck units themselves serve as the base units from which multiples or submultiples are derived.
The building blocks of latakama are these fundamental constants:
- $\hbar$, the [reduced Planck constant](https://en.wikipedia.org/wiki/Planck_constant#Reduced_Planck_constant)
- $G$, the [gravitational constant](https://en.wikipedia.org/wiki/Gravitational_constant)
- $c$, the [speed of light](https://en.wikipedia.org/wiki/Speed_of_light)
- $k_{\text{B}}$, the [Boltzmann constant](https://en.wikipedia.org/wiki/Boltzmann_constant)
- $\Lambda$, the [cosmological constant](https://en.wikipedia.org/wiki/Cosmological_constant)
## Unit prefixes
The unit prefixes indicate multiples or submultiples of a base unit. They are scaled by a factor or divisor of $2^{8*n}$.
## Base units
### la
The **la** represents the best possible resolution that any distance can be measured at or the minimum size that you can meaningfully ascribe to anything. The fundamental limit of the measurability of space.
$$
1 la = \sqrt{\frac{\hbar G}{c^{3}}}
$$
| Prefix | Factor | Conventional |
| --- | --- | --- |
| – | $2^{8*0}$ | $0.000016163\text{ quectometers}$ |
| ku | $2^{8*1}$ | $0.0041376\text{ quectometers}$ |
| je | $2^{8*2}$ | $1.0592\text{ quectometers}$ |
| po | $2^{8*3}$ | $0.27116\text{ rontometers}$ |
| ni | $2^{8*4}$ | $69.42\text{ rontometers}$ |
| tu | $2^{8*5}$ | $17.771\text{ yoctometers}$ |
| le | $2^{8*6}$ | $4.549\text{ zeptometers}$ |
| so | $2^{8*7}$ | $1.1646\text{ attometers}$ |
| ki | $2^{8*8}$ | $0.29815\text{ femtometers}$ |
| ju | $2^{8*9}$ | $76.33\text{ femtometers}$ |
| pe | $2^{8*10}$ | $19.539\text{ picometers}$ |
| no | $2^{8*11}$ | $5.002\text{ nanometers}$ |
| ti | $2^{8*12}$ | $1.2805\text{ micrometers}$ |
| lu | $2^{8*13}$ | $0.32782\text{ millimeters}$ |
| se | $2^{8*14}$ | $8.392\text{ centimeters}$ |
| mo | $2^{8*15}$ | $2.1484\text{ dekameters}$ |
| ji | $2^{8*16}$ | $5.500\text{ kilometers}$ |
| pu | $2^{8*17}$ | $4.696\text{ light milliseconds}$ |
| ne | $2^{8*18}$ | $5.042\text{ Jupiter equatorial radii}$ |
| to | $2^{8*19}$ | $5.130\text{ light minutes}$ |
| li | $2^{8*20}$ | $0.9120\text{ light days}$ |
| su | $2^{8*21}$ | $6.047\text{ petameters}$ |
| me | $2^{8*22}$ | $1.5481\text{ exameters}$ |
| ko | $2^{8*23}$ | $1.5\text{ galactic units}$ |
| pi | $2^{8*24}$ | $3.2879\text{ megaparsecs}$ |
| nu | $2^{8*25}$ | $2.7453\text{ gigalightyears}$ |
| te | $2^{8*26}$ | $6.649\text{ ronnameters}$ |
| lo | $2^{8*27}$ | $1.7021\text{ quettameters}$ |
| si | $2^{8*28}$ | $14.121\text{ petaparsecs}$ |
| mu | $2^{8*29}$ | $3.6151\text{ exaparsecs}$ |
| ke | $2^{8*30}$ | $925.5\text{ exaparsecs}$ |
| jo | $2^{8*31}$ | $236920\text{ exaparsecs}$ |
| kumi | $2^{8*32}$ | $6.065*10^{7}\text{ exaparsecs}$ |
| kuku | $2^{8*33}$ | $1.5527*10^{10}\text{ exaparsecs}$ |
| kuje | $2^{8*34}$ | $3.9748*10^{12}\text{ exaparsecs}$ |
| kupo | $2^{8*35}$ | $1.0176*10^{15}\text{ exaparsecs}$ |
| kuni | $2^{8*36}$ | $2.6049*10^{17}\text{ exaparsecs}$ |
| kutu | $2^{8*37}$ | $6.669*10^{19}\text{ exaparsecs}$ |
| kule | $2^{8*38}$ | $1.7072*10^{22}\text{ exaparsecs}$ |
| kuso | $2^{8*39}$ | $4.3704*10^{24}\text{ exaparsecs}$ |
| kuki | $2^{8*40}$ | $1.1188*10^{27}\text{ exaparsecs}$ |
| kuju | $2^{8*41}$ | $2.8642*10^{29}\text{ exaparsecs}$ |
| kupe | $2^{8*42}$ | $7.332*10^{31}\text{ exaparsecs}$ |
| kuno | $2^{8*43}$ | $1.8771*10^{34}\text{ exaparsecs}$ |
| kuti | $2^{8*44}$ | $4.805*10^{36}\text{ exaparsecs}$ |
| kulu | $2^{8*45}$ | $1.2301*10^{39}\text{ exaparsecs}$ |
| kuse | $2^{8*46}$ | $3.1492*10^{41}\text{ exaparsecs}$ |
| kumo | $2^{8*47}$ | $8.062*10^{43}\text{ exaparsecs}$ |
| kuji | $2^{8*48}$ | $2.0638*10^{46}\text{ exaparsecs}$ |
| kupu | $2^{8*49}$ | $5.283*10^{48}\text{ exaparsecs}$ |
| kune | $2^{8*50}$ | $1.3526*10^{51}\text{ exaparsecs}$ |
| kuto | $2^{8*51}$ | $3.4626*10^{53}\text{ exaparsecs}$ |
| kuli | $2^{8*52}$ | $8.864*10^{55}\text{ exaparsecs}$ |
| kusu | $2^{8*53}$ | $2.2692*10^{58}\text{ exaparsecs}$ |
| kume | $2^{8*54}$ | $5.809*10^{60}\text{ exaparsecs}$ |
| kuko | $2^{8*55}$ | $1.4872*10^{63}\text{ exaparsecs}$ |
| kupi | $2^{8*56}$ | $3.8071*10^{65}\text{ exaparsecs}$ |
| kunu | $2^{8*57}$ | $9.746*10^{67}\text{ exaparsecs}$ |
| kute | $2^{8*58}$ | $2.4950*10^{70}\text{ exaparsecs}$ |
| kulo | $2^{8*59}$ | $6.387*10^{72}\text{ exaparsecs}$ |
| kusi | $2^{8*60}$ | $1.6351*10^{75}\text{ exaparsecs}$ |
| kumu | $2^{8*61}$ | $4.1860*10^{77}\text{ exaparsecs}$ |
| kuke | $2^{8*62}$ | $1.0716*10^{80}\text{ exaparsecs}$ |
| kujo | $2^{8*63}$ | $2.7433*10^{82}\text{ exaparsecs}$ |
### ta
The **ta** is the time required for light to travel a distance of 1 [la](#la) in vacuum.
$$
1 ta = \frac{1 la}{c} = \frac{\sqrt{\frac{\hbar G}{c^{3}}}}{c} = \sqrt{\frac{\hbar G}{c^{5}}}
$$
| Prefix | Factor | Conventional |
| --- | --- | --- |
| – | $2^{8*0}$ | $5.391*10^{-14}\text{ quectoseconds}$ |
| ku | $2^{8*1}$ | $1.3802*10^{-11}\text{ quectoseconds}$ |
| je | $2^{8*2}$ | $3.5332*10^{-9}\text{ quectoseconds}$ |
| po | $2^{8*3}$ | $9.045*10^{-7}\text{ quectoseconds}$ |
| ni | $2^{8*4}$ | $0.00023155\text{ quectoseconds}$ |
| tu | $2^{8*5}$ | $0.05928\text{ quectoseconds}$ |
| le | $2^{8*6}$ | $15.175\text{ quectoseconds}$ |
| so | $2^{8*7}$ | $3.8848\text{ rontoseconds}$ |
| ki | $2^{8*8}$ | $0.9945\text{ yoctoseconds}$ |
| ju | $2^{8*9}$ | $0.25459\text{ zeptoseconds}$ |
| pe | $2^{8*10}$ | $65.18\text{ zeptoseconds}$ |
| no | $2^{8*11}$ | $16.685\text{ attoseconds}$ |
| ti | $2^{8*12}$ | $4.2714\text{ femtoseconds}$ |
| lu | $2^{8*13}$ | $1.0935\text{ picoseconds}$ |
| se | $2^{8*14}$ | $0.27993\text{ nanoseconds}$ |
| mo | $2^{8*15}$ | $71.66\text{ nanoseconds}$ |
| ji | $2^{8*16}$ | $18.345\text{ microseconds}$ |
| pu | $2^{8*17}$ | $4.696\text{ milliseconds}$ |
| ne | $2^{8*18}$ | $1.2023\text{ seconds}$ |
| to | $2^{8*19}$ | $5.130\text{ minutes}$ |
| li | $2^{8*20}$ | $0.9120\text{ days}$ |
| su | $2^{8*21}$ | $7.675\text{ months}$ |
| me | $2^{8*22}$ | $1.6363\text{ centuries}$ |
| ko | $2^{8*23}$ | $41.890\text{ millennia}$ |
| pi | $2^{8*24}$ | $10.731\text{ megayears}$ |
| nu | $2^{8*25}$ | $2.7471\text{ gigayears}$ |
| te | $2^{8*26}$ | $0.7033\text{ terayears}$ |
| lo | $2^{8*27}$ | $0.18004\text{ petayears}$ |
| si | $2^{8*28}$ | $46.09\text{ petayears}$ |
| mu | $2^{8*29}$ | $11.799\text{ exayears}$ |
| ke | $2^{8*30}$ | $3.0205\text{ zettayears}$ |
| jo | $2^{8*31}$ | $0.7733\text{ yottayears}$ |
| kumi | $2^{8*32}$ | $197.95\text{ yottayears}$ |
| kuku | $2^{8*33}$ | $50680\text{ yottayears}$ |
| kuje | $2^{8*34}$ | $1.2973*10^{7}\text{ yottayears}$ |
| kupo | $2^{8*35}$ | $3.3211*10^{9}\text{ yottayears}$ |
| kuni | $2^{8*36}$ | $8.502*10^{11}\text{ yottayears}$ |
| kutu | $2^{8*37}$ | $2.1765*10^{14}\text{ yottayears}$ |
| kule | $2^{8*38}$ | $5.572*10^{16}\text{ yottayears}$ |
| kuso | $2^{8*39}$ | $1.4264*10^{19}\text{ yottayears}$ |
| kuki | $2^{8*40}$ | $3.6516*10^{21}\text{ yottayears}$ |
| kuju | $2^{8*41}$ | $9.348*10^{23}\text{ yottayears}$ |
| kupe | $2^{8*42}$ | $2.3931*10^{26}\text{ yottayears}$ |
| kuno | $2^{8*43}$ | $6.126*10^{28}\text{ yottayears}$ |
| kuti | $2^{8*44}$ | $1.5683*10^{31}\text{ yottayears}$ |
| kulu | $2^{8*45}$ | $4.0150*10^{33}\text{ yottayears}$ |
| kuse | $2^{8*46}$ | $1.0278*10^{36}\text{ yottayears}$ |
| kumo | $2^{8*47}$ | $2.6312*10^{38}\text{ yottayears}$ |
| kuji | $2^{8*48}$ | $6.736*10^{40}\text{ yottayears}$ |
| kupu | $2^{8*49}$ | $1.7244*10^{43}\text{ yottayears}$ |
| kune | $2^{8*50}$ | $4.4145*10^{45}\text{ yottayears}$ |
| kuto | $2^{8*51}$ | $1.1301*10^{48}\text{ yottayears}$ |
| kuli | $2^{8*52}$ | $2.8931*10^{50}\text{ yottayears}$ |
| kusu | $2^{8*53}$ | $7.406*10^{52}\text{ yottayears}$ |
| kume | $2^{8*54}$ | $1.8960*10^{55}\text{ yottayears}$ |
| kuko | $2^{8*55}$ | $4.854*10^{57}\text{ yottayears}$ |
| kupi | $2^{8*56}$ | $1.2426*10^{60}\text{ yottayears}$ |
| kunu | $2^{8*57}$ | $3.1810*10^{62}\text{ yottayears}$ |
| kute | $2^{8*58}$ | $8.143*10^{64}\text{ yottayears}$ |
| kulo | $2^{8*59}$ | $2.0847*10^{67}\text{ yottayears}$ |
| kusi | $2^{8*60}$ | $5.337*10^{69}\text{ yottayears}$ |
| kumu | $2^{8*61}$ | $1.3662*10^{72}\text{ yottayears}$ |
| kuke | $2^{8*62}$ | $3.4975*10^{74}\text{ yottayears}$ |
| kujo | $2^{8*63}$ | $8.954*10^{76}\text{ yottayears}$ |
### ka
The **ka** is the temperature at which the wavelength of light emitted by thermal radiation reaches 1 [la](#la).
$$
1 ka = \sqrt{\frac{la^{10}}{G^2 k_{\text{B}}^2 ta^8}} = \sqrt{\frac{c^5 \hbar}{G k_{\text{B}}^2}}
$$
| Prefix | Divisor | Conventional |
| --- | --- | --- |
| ku | $2^{8*63}$ | $2.7051*10^{-90}\text{ quectokelvins}$ |
| je | $2^{8*62}$ | $6.925*10^{-88}\text{ quectokelvins}$ |
| po | $2^{8*61}$ | $1.7728*10^{-85}\text{ quectokelvins}$ |
| ni | $2^{8*60}$ | $4.538*10^{-83}\text{ quectokelvins}$ |
| tu | $2^{8*59}$ | $1.1618*10^{-80}\text{ quectokelvins}$ |
| le | $2^{8*58}$ | $2.9743*10^{-78}\text{ quectokelvins}$ |
| so | $2^{8*57}$ | $7.614*10^{-76}\text{ quectokelvins}$ |
| ki | $2^{8*56}$ | $1.9492*10^{-73}\text{ quectokelvins}$ |
| ju | $2^{8*55}$ | $4.990*10^{-71}\text{ quectokelvins}$ |
| pe | $2^{8*54}$ | $1.2775*10^{-68}\text{ quectokelvins}$ |
| no | $2^{8*53}$ | $3.2703*10^{-66}\text{ quectokelvins}$ |
| ti | $2^{8*52}$ | $8.372*10^{-64}\text{ quectokelvins}$ |
| lu | $2^{8*51}$ | $2.1432*10^{-61}\text{ quectokelvins}$ |
| se | $2^{8*50}$ | $5.487*10^{-59}\text{ quectokelvins}$ |
| mo | $2^{8*49}$ | $1.4046*10^{-56}\text{ quectokelvins}$ |
| ji | $2^{8*48}$ | $3.5957*10^{-54}\text{ quectokelvins}$ |
| pu | $2^{8*47}$ | $9.205*10^{-52}\text{ quectokelvins}$ |
| ne | $2^{8*46}$ | $2.3565*10^{-49}\text{ quectokelvins}$ |
| to | $2^{8*45}$ | $6.033*10^{-47}\text{ quectokelvins}$ |
| li | $2^{8*44}$ | $1.5443*10^{-44}\text{ quectokelvins}$ |
| su | $2^{8*43}$ | $3.9535*10^{-42}\text{ quectokelvins}$ |
| me | $2^{8*42}$ | $1.0121*10^{-39}\text{ quectokelvins}$ |
| ko | $2^{8*41}$ | $2.5910*10^{-37}\text{ quectokelvins}$ |
| pi | $2^{8*40}$ | $6.633*10^{-35}\text{ quectokelvins}$ |
| nu | $2^{8*39}$ | $1.6980*10^{-32}\text{ quectokelvins}$ |
| te | $2^{8*38}$ | $4.3470*10^{-30}\text{ quectokelvins}$ |
| lo | $2^{8*37}$ | $1.1128*10^{-27}\text{ quectokelvins}$ |
| si | $2^{8*36}$ | $2.8488*10^{-25}\text{ quectokelvins}$ |
| mu | $2^{8*35}$ | $7.293*10^{-23}\text{ quectokelvins}$ |
| ke | $2^{8*34}$ | $1.8670*10^{-20}\text{ quectokelvins}$ |
| jo | $2^{8*33}$ | $4.780*10^{-18}\text{ quectokelvins}$ |
| kumi | $2^{8*32}$ | $1.2236*10^{-15}\text{ quectokelvins}$ |
| kuku | $2^{8*31}$ | $3.1323*10^{-13}\text{ quectokelvins}$ |
| kuje | $2^{8*30}$ | $8.019*10^{-11}\text{ quectokelvins}$ |
| kupo | $2^{8*29}$ | $2.0528*10^{-8}\text{ quectokelvins}$ |
| kuni | $2^{8*28}$ | $5.255*10^{-6}\text{ quectokelvins}$ |
| kutu | $2^{8*27}$ | $0.0013453\text{ quectokelvins}$ |
| kule | $2^{8*26}$ | $0.34440\text{ quectokelvins}$ |
| kuso | $2^{8*25}$ | $0.08817\text{ rontokelvins}$ |
| kuki | $2^{8*24}$ | $22.571\text{ rontokelvins}$ |
| kuju | $2^{8*23}$ | $5.778\text{ yoctokelvins}$ |
| kupe | $2^{8*22}$ | $1.4792\text{ zeptokelvins}$ |
| kuno | $2^{8*21}$ | $0.37867\text{ attokelvins}$ |
| kuti | $2^{8*20}$ | $0.09694\text{ femtokelvins}$ |
| kulu | $2^{8*19}$ | $24.817\text{ femtokelvins}$ |
| kuse | $2^{8*18}$ | $6.353\text{ picokelvins}$ |
| kumo | $2^{8*17}$ | $1.6264\text{ nanokelvins}$ |
| kuji | $2^{8*16}$ | $0.41636\text{ microkelvins}$ |
| kupu | $2^{8*15}$ | $0.10659\text{ millikelvins}$ |
| kune | $2^{8*14}$ | $2.7286\text{ centikelvins}$ |
| kuto | $2^{8*13}$ | $6.985\text{ kelvins}$ |
| kuli | $2^{8*12}$ | $1.7882\text{ kilokelvins}$ |
| kusu | $2^{8*11}$ | $0.4578\text{ megakelvins}$ |
| kume | $2^{8*10}$ | $0.11719\text{ gigakelvins}$ |
| kuko | $2^{8*9}$ | $30.002\text{ gigakelvins}$ |
| kupi | $2^{8*8}$ | $7.680\text{ terakelvins}$ |
| kunu | $2^{8*7}$ | $1.9662\text{ petakelvins}$ |
| kute | $2^{8*6}$ | $0.5033\text{ exakelvins}$ |
| kulo | $2^{8*5}$ | $0.12886\text{ zettakelvins}$ |
| kusi | $2^{8*4}$ | $32.987\text{ zettakelvins}$ |
| kumu | $2^{8*3}$ | $8.445\text{ yotta kelvins}$ |
| kuke | $2^{8*2}$ | $2.1618\text{ ronnakelvins}$ |
| kujo | $2^{8*1}$ | $0.5534\text{ quettakelvins}$ |
| – | $2^{8*0}$ | $141.68\text{ quettakelvins}$ |
### ma
The **ma** is the cosmological-quantum point mass. It represents the theoretical mass scale at which gravitational, quantum mechanical, and cosmological effects become equally significant. At this scale, quantum uncertainty and universal expansion are balanced, serving as a fundamental reference for mass in quantum cosmology.
$$
1 ma = \frac{(\frac{la^{14} \Lambda}{G^4 ta^8})^{1/4}}{2^{3/4} \sqrt[4]{\pi}} = \frac{(\frac{\hbar^3 \Lambda}{c G})^{1/4}}{2^{3/4} \sqrt[4]{\pi}}
$$
| Prefix | Divisor | Conventional |
| --- | --- | --- |
| – | $2^{8*0}$ | $0.0022\text{ electronvolts per speed of light squared}$ |
| ku | $2^{8*1}$ | $0.58\text{ electronvolts per speed of light squared}$ |
| je | $2^{8*2}$ | $0.26\text{ quectograms}$ |
| po | $2^{8*3}$ | $38\text{ kiloelectronvolts per speed of light squared}$ |
| ni | $2^{8*4}$ | $17\text{ rontograms}$ |
| tu | $2^{8*5}$ | $2.7\text{ unified atomic mass units}$ |
| le | $2^{8*6}$ | $5.1\text{ Higgs boson masses}$ |
| so | $2^{8*7}$ | $0.29\text{ attograms}$ |
| ki | $2^{8*8}$ | $74\text{ attograms}$ |
| ju | $2^{8*9}$ | $19\text{ femtograms}$ |
| pe | $2^{8*10}$ | $4.8\text{ picograms}$ |
| no | $2^{8*11}$ | $1.24\text{ nanograms}$ |
| ti | $2^{8*12}$ | $0.32\text{ micrograms}$ |
| lu | $2^{8*13}$ | $3.7\text{ Planck masses}$ |
| se | $2^{8*14}$ | $2.1\text{ centigrams}$ |
| mo | $2^{8*15}$ | $5.3\text{ grams}$ |
| ji | $2^{8*16}$ | $1.4\text{ kilograms}$ |
| pu | $2^{8*17}$ | $0.35\text{ megagrams}$ |
| ne | $2^{8*18}$ | $0.089\text{ gigagrams}$ |
| to | $2^{8*19}$ | $23\text{ gigagrams}$ |
| li | $2^{8*20}$ | $5.9\text{ teragrams}$ |
| su | $2^{8*21}$ | $1.5\text{ petagrams}$ |
| me | $2^{8*22}$ | $0.38\text{ exagrams}$ |
| ko | $2^{8*23}$ | $0.098\text{ zettagrams}$ |
| pi | $2^{8*24}$ | $25\text{ zettagrams}$ |
| nu | $2^{8*25}$ | $6.4\text{ yottagrams}$ |
| te | $2^{8*26}$ | $2.6\text{ Mars masses}$ |
| lo | $2^{8*27}$ | $4.1\text{ Neptune masses}$ |
| si | $2^{8*28}$ | $57\text{ Jupiter masses}$ |
| mu | $2^{8*29}$ | $14\text{ solar masses}$ |
| ke | $2^{8*30}$ | $0.018\text{ gravity-seconds}$ |
| jo | $2^{8*31}$ | $4.5\text{ gravity-seconds}$ |
| kumi | $2^{8*32}$ | $0.0109\text{ galactic mass scales}$ |
| kuku | $2^{8*33}$ | $2.8\text{ galactic mass scales}$ |
| kuje | $2^{8*34}$ | $720\text{ galactic mass scales}$ |
| kupo | $2^{8*35}$ | $2\text{ horizon mass scales at equality}$ |
| kuni | $2^{8*36}$ | $500\text{ horizon mass scales at equality}$ |
| kutu | $2^{8*37}$ | $0.003\text{ universe masses (ordinary matter)}$ |
| kule | $2^{8*38}$ | $0.9\text{ universe masses (ordinary matter)}$ |
| kuso | $2^{8*39}$ | $32\text{ vacuum dominated universe mass scales}$ |
| kuki | $2^{8*40}$ | $8000\text{ vacuum dominated universe mass scales}$ |
| kuju | $2^{8*41}$ | $2.1*10^{6}\text{ vacuum dominated universe mass scales}$ |
| kupe | $2^{8*42}$ | $5*10^{8}\text{ vacuum dominated universe mass scales}$ |
| kuno | $2^{8*43}$ | $1.4*10^{11}\text{ vacuum dominated universe mass scales}$ |
| kuti | $2^{8*44}$ | $3.6*10^{13}\text{ vacuum dominated universe mass scales}$ |
| kulu | $2^{8*45}$ | $9*10^{15}\text{ vacuum dominated universe mass scales}$ |
| kuse | $2^{8*46}$ | $2.3*10^{18}\text{ vacuum dominated universe mass scales}$ |
| kumo | $2^{8*47}$ | $6*10^{20}\text{ vacuum dominated universe mass scales}$ |
| kuji | $2^{8*48}$ | $1.5*10^{23}\text{ vacuum dominated universe mass scales}$ |
| kupu | $2^{8*49}$ | $3.9*10^{25}\text{ vacuum dominated universe mass scales}$ |
| kune | $2^{8*50}$ | $1.0*10^{28}\text{ vacuum dominated universe mass scales}$ |
| kuto | $2^{8*51}$ | $2.6*10^{30}\text{ vacuum dominated universe mass scales}$ |
| kuli | $2^{8*52}$ | $7*10^{32}\text{ vacuum dominated universe mass scales}$ |
| kusu | $2^{8*53}$ | $1.7*10^{35}\text{ vacuum dominated universe mass scales}$ |
| kume | $2^{8*54}$ | $4.3*10^{37}\text{ vacuum dominated universe mass scales}$ |
| kuko | $2^{8*55}$ | $1.1*10^{40}\text{ vacuum dominated universe mass scales}$ |
| kupi | $2^{8*56}$ | $2.8*10^{42}\text{ vacuum dominated universe mass scales}$ |
| kunu | $2^{8*57}$ | $7*10^{44}\text{ vacuum dominated universe mass scales}$ |
| kute | $2^{8*58}$ | $1.8*10^{47}\text{ vacuum dominated universe mass scales}$ |
| kulo | $2^{8*59}$ | $5*10^{49}\text{ vacuum dominated universe mass scales}$ |
| kusi | $2^{8*60}$ | $1.2*10^{52}\text{ vacuum dominated universe mass scales}$ |
| kumu | $2^{8*61}$ | $3.1*10^{54}\text{ vacuum dominated universe mass scales}$ |
| kuke | $2^{8*62}$ | $8*10^{56}\text{ vacuum dominated universe mass scales}$ |
| kujo | $2^{8*63}$ | $2.0*10^{59}\text{ vacuum dominated universe mass scales}$ |