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C 6

Carbon (C)

nonmetal
Periodo: 2 Gruppo: 14 Blocco: p

Solid

Peso atomico standard

12,011 u [12,0096, 12,0116]

Configurazione elettronica

[He] 2s2 2p2

Punto di fusione

3549,85 °C

Punto di ebollizione

3824,85 °C

Densità

2267 kg/m³

Stati di ossidazione

−4, −3, −2, −1, 0, +1, +2, +3, +4

Elettronegatività (Pauling)

2,55

Energia di ionizzazione (1ª)

11,260288 eV

Anno della scoperta

1797

Raggio atomico

70 pm

Dettagli

Origine del nome Latin: carbo, (charcoal).
Scopritori Known to the ancients

Carbon is a nonmetal in group 14 and the defining element of organic chemistry. Its small atoms form strong covalent bonds with carbon and many other elements, allowing chains, rings, networks, and multiple bonds of great diversity. It occurs naturally as graphite, diamond, amorphous carbon-rich materials, carbonate minerals, fossil carbon, dissolved carbon species, and as a central element in living matter.

Carbon is a member of group 14 of the periodic table. It has three allotropic forms of it, diamonds, graphite and fullerite. Carbon-14 is commonly used in radioactive dating. Carbon occurs in all organic life and is the basis of organic chemistry. Carbon has the interesting chemical property of being able to bond with itself, and a wide variety of other elements.

The name derives from the Latin carbo for "charcoal". It was known in prehistoric times in the form of charcoal and soot. In 1797, the English chemist Smithson Tennant proved that diamond is pure carbon.

Carbon, the sixth most abundant element in the universe, has been known since ancient times. Carbon is most commonly obtained from coal deposits, although it usually must be processed into a form suitable for commercial use. Three naturally occurring allotropes of carbon are known to exist: amorphous, graphite and diamond.

From the Latin word carbo: charcoal. Carbon, an element of prehistoric discovery, is very widely distributed in nature. It is found in abundance in the sun, stars, comets, and atmospheres of most planets. Carbon in the form of microscopic diamonds is found in some meteorites.

Natural diamonds are found in kimberlite of ancient volcanic "pipes," found in South Africa, Arkansas, and elsewhere. Diamonds are now also being recovered from the ocean floor off the Cape of Good Hope. About 30% of all industrial diamonds used in the U.S. are now made synthetically.

The energy of the sun and stars can be attributed at least in part to the well-known carbon-nitrogen cycle.

Immagini

Proprietà

Chimiche

Elettronegatività (Pauling)
2,55 Confronta Elettronegatività (Pauling) di tutti gli elementi →
Elettronegatività (Allen)
2,544
Affinità elettronica
1,2621 eV
Energia di ionizzazione (1ª)
11,260288 eV Confronta Energia di ionizzazione (1ª) di tutti gli elementi →
Energia di ionizzazione (2ª)
24,383227 eV Confronta Energia di ionizzazione (2ª) di tutti gli elementi →
Energia di ionizzazione (3ª)
47,887945 eV Confronta Energia di ionizzazione (3ª) di tutti gli elementi →
Energia di ionizzazione (4ª)
64,493742 eV Confronta Energia di ionizzazione (4ª) di tutti gli elementi →
Energia di ionizzazione (5ª)
392,09191 eV Confronta Energia di ionizzazione (5ª) di tutti gli elementi →
Stati di ossidazione
−4, −3, −2, −1, 0, +1, +2, +3, +4 Confronta Stati di ossidazione di tutti gli elementi →
Elettroni di valenza
4 Confronta Elettroni di valenza di tutti gli elementi →
Allotropi
["graphite"]
Configurazione elettronica
[He] 2s2 2p2

Termodinamiche

Punto triplo (temperatura)
4489 °C
Punto triplo (pressione)
1,03e+7 Pa
Calore di vaporizzazione
7,410478 eV Confronta Calore di vaporizzazione di tutti gli elementi →
Calore di sublimazione
7,42789 eV
Calore di atomizzazione
7,42789 eV
Entalpia di atomizzazione
7,42986 eV

Struttura cristallina

Costante reticolare a
357 pm

Struttura elettronica

Elettroni per guscio
2, 4 Confronta Elettroni per guscio di tutti gli elementi →

Identificativi

Numero CAS
7440-44-0 Confronta Numero CAS di tutti gli elementi →
Simbolo di termine
3P0
InChI
InChI=1S/C
Chiave InChI
OKTJSMMVPCPJKN-UHFFFAOYSA-N

Configurazione elettronica Misurato

Carica ionica
Protoni 6
Elettroni 6
Carica Neutro
Configurazione C: 2s² 2p²
Configurazione elettronica
Misurato
[He] 2s² 2p²
1s² 2s² 2p²
Diagramma degli orbitali
1s
2/2
2s
2/2
2p
2/6 2↑
Elettroni totali: 6 Spaiati: 2 ?

Modello atomico

Protoni 6
Neutroni 6
Elettroni 6
Numero di massa 12
Stabilità Stabile

Gli isotopi modificano il numero di neutroni, la massa e la stabilità — non la configurazione elettronica di un atomo neutro.

Modello atomico schematico, non in scala.

Impronta atomica

Spettro di emissione / assorbimento

25 / 50 (50 50 con intensità)
Misurato
Emissione Visibile: 380–750 nm

Distribuzione isotopica

1298,9300%131,0700%Numero di massaAbbondanza naturale (%)
Numero di massaMassa atomica (u)Abbondanza naturaleEmivita
12 Stabile1298,9300%Stabile
13 Stabile13,00335483507 ± 0,000000000231,0700%Stabile
Misurato

Fase / Stato

1 atm / 101,325 kPa
Solido 25 °C (298,15 K)

Motivo: 3799,8 °C sotto il punto di sublimazione (3824,85 °C)

Punto di sublimazione 3824,85 °C
0 K Temperatura attuale: 25 °C 6000 K
Sequenza delle fasi

Schema non in scala

Solido
Gas
Sublimazione
25°C
Solido
Liquido
Gas
Attuale

Punti di transizione di fase

Punto di sublimazione Letteratura
3824,85 °C
Fase attuale Calcolato
Solido

Energie di transizione

Calore di vaporizzazione Letteratura
7,410478 eV

Energia necessaria per vaporizzare 1 mol al punto di ebollizione

Calore di sublimazione Letteratura
7,42789 eV

Energia necessaria per sublimare 1 mol al punto di sublimazione

Densità

Densità di riferimento Letteratura
2267 kg/m³

In condizioni standard

Densità attuale Calcolato
2267 kg/m³

In condizioni standard

Avanzate

Punto triplo Letteratura
4489 °C

Spettri atomici

Sono visualizzati 10 di 11. Ordinamento per carica ionica crescente.

Righe disponibili ?

IoneCaricaRighe totaliProbabilità di transizioneDesignazioni dei livelli
C I 0210216162102
12C I Isotopo089089
13C I Isotopo089089
12C II Isotopo+11870187
14C II Isotopo+11870187
C II +1160514331605
13C II Isotopo+11870187
C III +2882878878
C IV +3259224255
C V +4149146147
Righe disponibili nel NIST →

Livelli disponibili ?

IoneCaricaLivelli
C I 0435
12C I Isotopo033
13C I Isotopo033
12C II Isotopo+136
14C II Isotopo+136
C II +1415
13C II Isotopo+136
C III +2201
C IV +3107
C V +4156
Livelli disponibili nel NIST →
6 C 12.0106

Carbon — Visualizzatore degli orbitali atomici

[He]2s22p2
Livelli energetici 2 4
Stati di ossidazione -4, -3, -2, -1, 0, +1, +2, +3, +4
HOMO 2p n=2 · l=1 · m=-1
Carbon — Anteprima del visualizzatore degli orbitali atomici
Three.js viene caricato soltanto su richiesta
6 C 12.0106

Carbon — Visualizzatore della struttura cristallina

Face-Centered Cubic · Pearson cF8
Sperimentale
Pearson cF8
N. coord. 4
Impacchettamento 34.000%
Carbon — Anteprima del visualizzatore della struttura cristallina
Three.js viene caricato soltanto su richiesta

Raggi ionici

CaricaCoordinazioneSpinRaggio
+44N/D15 pm
+46N/D16 pm

Composti

C
12,011 u

Isotopi (2)

Carbon has seven isotopes. In 1961 the International Union of Pure and Applied Chemistry adopted the isotope carbon-12 as the basis for atomic weights. Carbon-14, an isotope with a half-life of 5715 years, has been widely used to date such materials as wood, archaeological specimens, etc.

Numero di massaMassa atomica (u)Abbondanza naturaleEmivitaModalità di decadimento
12 Stabile1298,9300% ± 0,0800%Stabile
stable
13 Stabile13,00335483507 ± 0,000000000231,0700% ± 0,0800%Stabile
stable
12 Stabile
Massa atomica (u) 12
Abbondanza naturale 98,9300% ± 0,0800%
Emivita Stabile
Modalità di decadimento
stable
13 Stabile
Massa atomica (u) 13,00335483507 ± 0,00000000023
Abbondanza naturale 1,0700% ± 0,0800%
Emivita Stabile
Modalità di decadimento
stable

Righe spettrali

Sono visualizzati 50 di 993. Per impostazione predefinita sono mostrate soltanto le righe spettrali con intensità misurata.

Lunghezza d'onda (nm)IntensitàStadio di ionizzazioneTipoTransizioneAccuratezzaFonte
505.214927 nm160000C Iemission2s2.2p.3s 1P* → 2s2.2p.4p 1DMisurataNIST
538.033014 nm120000C Iemission2s2.2p.3s 1P* → 2s2.2p.4p 1PMisurataNIST
711.31656 nm110000C Iemission2s2.2p.3p 3D → 2s2.2p.4d 3F*MisurataNIST
493.202524 nm73000C Iemission2s2.2p.3s 1P* → 2s2.2p.4p 1SMisurataNIST
477.173374 nm69000C Iemission2s2.2p.3s 3P* → 2s2.2p.4p 3PMisurataNIST
711.697758 nm45000C Iemission2s2.2p.3p 3D → 2s2.2p.5s 3P*MisurataNIST
658.76211 nm40000C Iemission2s2.2p.3p 1P → 2s2.2p.4d 1P*MisurataNIST
579.311495 nm38000C Iemission2s.2p3 3D* → 2s2.2p.4p 3PMisurataNIST
711.96559 nm37000C Iemission2s2.2p.3p 3D → 2s2.2p.5s 3P*MisurataNIST
580.059993 nm35000C Iemission2s.2p3 3D* → 2s2.2p.4p 3PMisurataNIST
600.1123 nm35000C Iemission2s2.2p.3p 3D → 2s2.2p.6s 3P*MisurataNIST
477.589266 nm34000C Iemission2s2.2p.3s 3P* → 2s2.2p.4p 3PMisurataNIST
437.13814 nm33000C Iemission2s2.2p.3s 1P* → 2s2.2p.5p 1PMisurataNIST
711.145795 nm32000C Iemission2s2.2p.3p 3D → 2s2.2p.4d 3F*MisurataNIST
682.814076 nm27000C Iemission2s2.2p.3p 1P → 2s2.2p.4d 1D*MisurataNIST
504.149039 nm25000C Iemission2s.2p3 3D* → 2s2.2p.(2P*<1/2>).4f 2[5/2]MisurataNIST
477.002376 nm24000C Iemission2s2.2p.3s 3P* → 2s2.2p.4p 3PMisurataNIST
600.6012 nm23000C Iemission2s2.2p.3p 3D → 2s2.2p.5d 3D*MisurataNIST
665.55294 nm20000C Iemission2s2.2p.3p 1P → 2s2.2p.5s 1P*MisurataNIST
710.011312 nm19000C Iemission2s2.2p.3p 3D → 2s2.2p.5s 3P*MisurataNIST
566.894 nm18000C Iemission2s2.2p.3p 1P → 2s2.2p.5d 1P*MisurataNIST
596.933151 nm18000C Iemission2s.2p3 3D* → 2s2.2p.4p 3DMisurataNIST
708.782188 nm18000C Iemission2s2.2p.3p 3D → 2s2.2p.4d 3D*MisurataNIST
402.94119 nm16000C Iemission2s2.2p.3s 3P* → 2s2.2p.5p 3PMisurataNIST
601.64487 nm16000C Iemission2s2.2p.3p 3D → 2s2.2p.5d 3F*MisurataNIST
473.426281 nm15000C Iemission2s.2p3 3D* → 2s2.2p.5p 3PMisurataNIST
481.737213 nm15000C Iemission2s2.2p.3s 3P* → 2s2.2p.4p 3SMisurataNIST
579.446608 nm15000C Iemission2s.2p3 3D* → 2s2.2p.4p 3PMisurataNIST
748.344451 nm15000C Iemission2s2.2p.3p 3S → 2s2.2p.4d 3P*MisurataNIST
406.52425 nm14000C Iemission2s2.2p.3s 3P* → 2s2.2p.5p 3DMisurataNIST
580.52017 nm14000C Iemission2s.2p3 3D* → 2s2.2p.4p 3PMisurataNIST
601.4833 nm14000C Iemission2s2.2p.3p 3D → 2s2.2p.6s 3P*MisurataNIST
710.89263 nm14000C Iemission2s2.2p.3p 3D → 2s2.2p.5s 3P*MisurataNIST
400.9928 nm13000C Iemission2s2.2p.3s 1P* → 2s2.2p.6p 1PMisurataNIST
422.83269 nm13000C Iemission2s2.2p.3s 1P* → 2s2.2p.5p 1SMisurataNIST
447.85821 nm13000C Iemission2s.2p3 3D* → 2s2.2p.(2P*<1/2>).5f 2[5/2]MisurataNIST
504.012903 nm12000C Iemission2s.2p3 3D* → 2s2.2p.(2P*<1/2>).4f 2[7/2]MisurataNIST
601.0669 nm12000C Iemission2s2.2p.3p 3D → 2s2.2p.6s 3P*MisurataNIST
406.4264 nm11000C Iemission2s2.2p.3s 3P* → 2s2.2p.5p 3DMisurataNIST
639.7965 nm11000C Iemission2s2.2p.3p 3S → 2s2.2p.6s 3P*MisurataNIST
666.3043 nm11000C Iemission2s2.2p.3p 3P → 2s2.2p.5d 3D*MisurataNIST
667.1849 nm11000C Iemission2s2.2p.3p 3P → 2s2.2p.6s 3P*MisurataNIST
403.180216 nm10000C Iemission2s2.2p.3s 3P* → 2s2.2p.5p 3PMisurataNIST
482.679468 nm10000C Iemission2s2.2p.3s 3P* → 2s2.2p.4p 3SMisurataNIST
598.903753 nm10000C Iemission2s.2p3 3D* → 2s2.2p.4p 3DMisurataNIST
707.649944 nm9900C Iemission2s2.2p.3p 3D → 2s2.2p.4d 3D*MisurataNIST
402.284321 nm9700C Iemission2s2.2p.3s 3P* → 2s2.2p.5p 3PMisurataNIST
555.1578 nm9600C Iemission2s2.2p.3p 3D → 2s2.2p.7s 3P*MisurataNIST
600.7173 nm9600C Iemission2s2.2p.3p 3D → 2s2.2p.6s 3P*MisurataNIST
502.492938 nm9400C Iemission2s.2p3 3D* → 2s2.2p.(2P*<3/2>).4f 2[7/2]MisurataNIST

Proprietà estese

Raggi covalenti (dati estesi)

Raggio covalente (Pyykkö)
75 pm
Raggio covalente (Pyykkö, legame doppio)
67 pm
Raggio covalente (Pyykkö, legame triplo)
60 pm
Raggio covalente (Bragg)
77 pm

Raggi di van der Waals

Bondi
170 pm
Batsanov
170 pm
Alvarez
177 pm
UFF
385,1 pm
MM3
204 pm
Dreiding
389,83 pm
Rowland–Taylor
177 pm

Raggi atomici e metallici

Raggio atomico (Rahm)
190 pm
Raggio metallico (C12)
86 pm

Scale di numerazione

Mendeleev
87
Pettifor
95
Glawe
87

Scale di elettronegatività

Ghosh
0
Miedema
6
Gunnarsson–Lundqvist
7
Robles–Bartolotti
6

Polarizzabilità e dispersione

Polarizzabilità dipolare
11,3 a.u.
Polarizzabilità dipolare (inc.)
0,2 a.u.
C₆
46,6 Ha·Bohr6
C₆ (Gould–Bučko)
47,9 Ha·Bohr6

Parametri di Miedema

Volume molare di Miedema
3,26 cm3/mol
Densità elettronica di Miedema
6

Rischio di approvvigionamento ed economia

Concentrazione della produzione
46
Rischio relativo di approvvigionamento
5
Distribuzione delle riserve
28
Stabilità politica (principale produttore)
24
Stabilità politica (principale detentore di riserve)
57

Transizioni di fase e allotropi

graphite Sublimazione
Punto di ebollizione4098,15 K
Punto triplo (temperatura)4762,15 K
Punto triplo (pressione)10300 kPa

Categorie degli stati di ossidazione

−1 extended
−2 extended
0 extended
+1 extended
+4 main
−4 main
+2 extended
+3 extended
−3 extended

Dati di riferimento avanzati

Costanti di schermaggio (3)
nOrbitaleσ
1s0,3273
2p2,8642
2s2,7834
Dettaglio dei raggi cristallini (3)
CaricaCNSpinrcrystal (pm)Origine
4III6
4IV29Pauling's (1960) crystal radius,
4VI30Ahrens (1952) ionic radius,
Modalità di decadimento degli isotopi (27)
IsotopoModalitàIntensità
82p100%
9B+100%
9B+p7,5%
9B+A38,4%
10B+100%
11B+100%
14B-100%
15B-100%
16B-100%
16B-n99%
Fattori di diffusione dei raggi X (502)
Energia (eV)f₁f₂
10—0,80688
10,1617—0,85152
10,3261—0,89863
10,4931—0,94834
10,6628—1,0008
10,8353—1,05755
11,0106—1,12167
11,1886—1,18968
11,3696—1,26181
11,5535—1,33832

Dati aggiuntivi

Isotopes in Forensic Science and Anthropology

Information on the use of this element's isotopes in forensic science and anthropology.

Variations in the isotope-amount ratio n(13C)/n(12C) of biological products can be observed using isotope-ratio mass spectrometry (IRMS) to detect adulteration (the addition of inferior ingredients) in honey and other food products.

The isotope-amount ratio n(13C)/n(12C) can fluctuate between carbon sources, for example C3 plants (found in temperate climates and which use atmospheric carbon dioxide to make a 3-carbon molecule during photosynthesis — examples include rice, potatoes, tomatoes, and sugar beets), C4 plants (found in hot climates and which use atmospheric carbon dioxide to make a 4-carbon molecule during photosynthesis — examples include corn and sugar cane), animal carbon, atmospheric CO2, etc. This commonly makes it possible to detect whether these different carbon sources have been mixed by using isotope or mass balance to distinguish, for example, between beet sugar and cane sugar. Complications in source identification can arise with plants that open stomata at night to collect carbon dioxide to use a third mechanism to fix atmospheric carbon dioxide (CAM or crassulacean acid metabolism). The isotope-amount ratio n(13C)/n(12C) of CAM plants overlaps that of C3 or C4 plants — examples include pineapples and jade plants. The following adulterations are commonly detected using stable carbon isotope IRMS:

–Variations in the isotope-amount ratio n(13C)/n(12C) of honey are used to detect the addition (and potential adulteration) of high fructose corn syrup, corn, or sugar cane [67] C. Cordella, I. Moussa, A. C. Martel, N. Sbirrazzuoli, L. Lizzani-Cuvelier. J. Agric. Food. Chem.50, 1751 (2002)..

–Variations in the isotope-amount ratio n(13C)/n(12C) of fruit juice have been used to detect the addition of a sugar [67] C. Cordella, I. Moussa, A. C. Martel, N. Sbirrazzuoli, L. Lizzani-Cuvelier. J. Agric. Food. Chem.50, 1751 (2002)..

–Variations in the isotope-amount ratio n(13C)/n(12C) of natural vanilla extract have been used to detect the addition of artificial vanillin or p-hydroxybenzaldehyde [67] C. Cordella, I. Moussa, A. C. Martel, N. Sbirrazzuoli, L. Lizzani-Cuvelier. J. Agric. Food. Chem.50, 1751 (2002)..

–Variations in the isotope-amount ratio n(13C)/n(12C) of beer are used to detect C4 carbon, which would indicate that a beer company may have added ingredients that are not traditionally used in brewing beer. Therefore, this ratio is used to detect the misrepresentation of a product as being pure [67] C. Cordella, I. Moussa, A. C. Martel, N. Sbirrazzuoli, L. Lizzani-Cuvelier. J. Agric. Food. Chem.50, 1751 (2002)., [68] J. R. Brooks, N. Buchmann, S. Phillips, B. Ehleringer, R. D. Evans, M. Lott, L. A. Martinelli, W. T. Pockman, D. Sandquist, J. P. Sparks, L. Sperry, D. Williams, J. R. Ehleringer. J. Agric. Food. Chem.50, 6413 (2002)..

Stable carbon IRMS has been used to determine if the botanical origin of an alcoholic spirit has been mislabeled and if chaptalization (the process of adding sugar to increase the alcoholic content) of wine has occurred [67] C. Cordella, I. Moussa, A. C. Martel, N. Sbirrazzuoli, L. Lizzani-Cuvelier. J. Agric. Food. Chem.50, 1751 (2002)., [68] J. R. Brooks, N. Buchmann, S. Phillips, B. Ehleringer, R. D. Evans, M. Lott, L. A. Martinelli, W. T. Pockman, D. Sandquist, J. P. Sparks, L. Sperry, D. Williams, J. R. Ehleringer. J. Agric. Food. Chem.50, 6413 (2002).. 14C scintillation counting has been used to determine the age of wine and alcoholic spirits [67] C. Cordella, I. Moussa, A. C. Martel, N. Sbirrazzuoli, L. Lizzani-Cuvelier. J. Agric. Food. Chem.50, 1751 (2002)., [68] J. R. Brooks, N. Buchmann, S. Phillips, B. Ehleringer, R. D. Evans, M. Lott, L. A. Martinelli, W. T. Pockman, D. Sandquist, J. P. Sparks, L. Sperry, D. Williams, J. R. Ehleringer. J. Agric. Food. Chem.50, 6413 (2002).. Variations in the isotope-amount ratio n(13C)/n(12C) of urine has been used to determine if steroids in urine are natural or of synthetic origin. These measurements enable anti-doping laboratories to perfect their methods for detecting steroid doping in athletes [69] B. D. Ahrens, A. W. Butch. Drug Test Anal.5, 534 (2013)., [70] E. Bulska, D. Gorczyca, I. Zalewska, A. Pokrywka, D. Kwiatkowska. J. Pharm. Biomed. Anal.106, 159 (2015)., [71] A. Casilli, T. Piper, F. A. de Oliveira, M. Costa Padilha, H. Marcelo Pereira, M. Thevis, F. R. de Aquino Neto. Drug Test Anal.8, 1204 (2016).. Variations in the isotope-amount ratio n(13C)/n(12C) of marijuana can provide information to determine if the plants were grown “inside” a building or greenhouse or were “open grown” (Fig. IUPAC.6.4). Plant carbon isotopic compositions are controlled by atmospheric CO2 and the supply and demand of CO2 in photosynthesis (the process used by plants to convert light energy from the sun into chemical energy). “Open grown” plants are grown in an area that is well ventilated and receives natural CO2. In contrast, plants grown “inside” receive supplemented CO2 and the photosynthesis process is more confined. Additionally, CO2 from a tank of compressed gas used to augment atmospheric CO2 to increase the growth of marijuana plants is commonly highly depleted in 13C as a refinery by-product. These differences change the carbon isotope ratios of the plants and the ratios vary enough to enable the determination of the growing and cultivation process of marijuana [72] E. K. Shibuya, J. E. Souza Sarkis, O. N. Neto, M. Z. Moreira, R. L. Victoria. Forensic Sci. Int.160, 35 (2006)., [73] J. B. West, J. M. Hurley, J. R. Ehleringer. J Forensic Sci.54, 84 (2009)..

Riferimenti (9)
  • [67] C. Cordella, I. Moussa, A. C. Martel, N. Sbirrazzuoli, L. Lizzani-Cuvelier. J. Agric. Food. Chem.50, 1751 (2002).
  • [68] J. R. Brooks, N. Buchmann, S. Phillips, B. Ehleringer, R. D. Evans, M. Lott, L. A. Martinelli, W. T. Pockman, D. Sandquist, J. P. Sparks, L. Sperry, D. Williams, J. R. Ehleringer. J. Agric. Food. Chem.50, 6413 (2002).
  • [69] B. D. Ahrens, A. W. Butch. Drug Test Anal.5, 534 (2013).
  • [70] E. Bulska, D. Gorczyca, I. Zalewska, A. Pokrywka, D. Kwiatkowska. J. Pharm. Biomed. Anal.106, 159 (2015).
  • [71] A. Casilli, T. Piper, F. A. de Oliveira, M. Costa Padilha, H. Marcelo Pereira, M. Thevis, F. R. de Aquino Neto. Drug Test Anal.8, 1204 (2016).
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Riferimenti

(9)
2 Atomic Mass Data Center (AMDC), International Atomic Energy Agency (IAEA)
C

The half-life and atomic mass data was provided by the Atomic Mass Data Center at the International Atomic Energy Agency.

3 IUPAC Commission on Isotopic Abundances and Atomic Weights (CIAAW)
Carbon

Element data are cited from the Atomic weights of the elements (an IUPAC Technical Report). The IUPAC periodic table of elements can be found at https://iupac.org/what-we-do/periodic-table-of-elements/. Additional information can be found within IUPAC publication doi:10.1515/pac-2015-0703 Copyright © 2020 International Union of Pure and Applied Chemistry.

4 IUPAC Periodic Table of the Elements and Isotopes (IPTEI)

The information are cited from Pure Appl. Chem. 2018; 90(12): 1833-2092, https://doi.org/10.1515/pac-2015-0703.

Nota sulla licenza: Copyright (c) 2020 International Union of Pure and Applied Chemistry. The International Union of Pure and Applied Chemistry (IUPAC) contribution within Pubchem is provided under a CC-BY-NC-ND 4.0 license, unless otherwise stated.
5 Jefferson Lab, U.S. Department of Energy
Carbon

Thomas Jefferson National Accelerator Facility (Jefferson Lab) is one of 17 national laboratories funded by the U.S. Department of Energy. The lab's primary mission is to conduct basic research of the atom's nucleus using the lab's unique particle accelerator, known as the Continuous Electron Beam Accelerator Facility (CEBAF). For more information visit https://www.jlab.org/

Nota sulla licenza: Please see citation and linking information: https://education.jlab.org/faq/index.html
6 Los Alamos National Laboratory, U.S. Department of Energy
Carbon

The periodic table at the LANL (Los Alamos National Laboratory) contains basic element information together with the history, source, properties, use, handling and more. The provenance data may be found from the link under the source name.

7 NIST Physical Measurement Laboratory
Carbon

The periodic table contains NIST's critically-evaluated data on atomic properties of the elements. The provenance data that include data for atomic spectroscopy, X-ray and gamma ray, radiation dosimetry, nuclear physics, and condensed matter physics may be found from the link under the source name. Ref: https://www.nist.gov/pml/atomic-spectra-database

8 PubChem Elements
Carbon

This section provides all form of data related to element Carbon.

9 PubChem Elements
Carbon

The element property data was retrieved from publications.

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