Nuclear Fusion - Revision history

NRJC at 13:35, 22 January 2021

2021-01-22T13:35:36Z

Ellen References at 07:37, 15 December 2019

2019-12-15T07:37:20Z

Ellen References at 18:37, 23 November 2019

2019-11-23T18:37:58Z

Ellen References at 14:40, 10 November 2019

2019-11-10T14:40:53Z

NRJC at 11:23, 19 July 2019

2019-07-19T11:23:30Z

NRJC at 08:27, 8 April 2019

2019-04-08T08:27:15Z

NRJC at 13:39, 11 March 2019

2019-03-11T13:39:48Z

NRJC at 13:36, 11 March 2019

2019-03-11T13:36:11Z

NRJC at 13:35, 11 March 2019

2019-03-11T13:35:29Z

NRJC at 13:34, 11 March 2019

2019-03-11T13:34:48Z

@@ Line 27: / Line 27: @@
 |-
 | style="height:20px; width:500px; text-align:center;" |'''Fusion''' of two [[Hydrogen]] [[Atomic Nucleus|nuclei]] ([[proton]]s) produces a [[Deuterium]] [[Atomic Nucleus|nucleus]].
-<math>{}_1^1H + {}_1^1H \rightarrow {}_1^2H + {}_{-1}^0\beta</math>
+<math>{}_1^1H + {}_1^1H \rightarrow {}_1^2H + {}_{+1}^0\beta</math>
 |}
@@ Line 35: / Line 35: @@
 |-
 | style="height:20px; width:500px; text-align:center;" |'''Fusion''' of a [[Hydrogen]] [[Atomic Nucleus|nucleus]] ([[proton]]) and a [[Deuterium]] [[Atomic Nucleus|nucleus]] produces a [[Tritium]] [[Atomic Nucleus|nucleus]].
-<math>{}_1^1H + {}_1^2H \rightarrow {}_1^3H + {}_{-1}^0\beta</math>
+<math>{}_1^1H + {}_1^2H \rightarrow {}_1^3H + {}_{+1}^0\beta</math>
 |}

← Older revision		Revision as of 07:37, 15 December 2019
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	:[https://www.amazon.co.uk/gp/product/1782945733/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1782945733&linkCode=as2&tag=nrjc-21&linkId=2a2dbec9db6bf5766c0458d908fa0a52 ''Nuclear fusion, page 58, GCSE Physics; The Revision Guide, CGP, Edexcel '']		:[https://www.amazon.co.uk/gp/product/1782945733/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1782945733&linkCode=as2&tag=nrjc-21&linkId=2a2dbec9db6bf5766c0458d908fa0a52 ''Nuclear fusion, page 58, GCSE Physics; The Revision Guide, CGP, Edexcel '']
	:[https://www.amazon.co.uk/gp/product/1292120223/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1292120223&linkCode=as2&tag=nrjc-21&linkId=068ecf40278c32406a7f1c6e66751417 ''Nuclear fusion, pages 110, 114-115, GCSE Physics, Pearson Edexcel '']		:[https://www.amazon.co.uk/gp/product/1292120223/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1292120223&linkCode=as2&tag=nrjc-21&linkId=068ecf40278c32406a7f1c6e66751417 ''Nuclear fusion, pages 110, 114-115, GCSE Physics, Pearson Edexcel '']
		+
		+	====OCR====
		+	:[https://www.amazon.co.uk/gp/product/0198359837/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=0198359837&linkCode=as2&tag=nrjc-21&linkId=3c4229e8b023b2b60768e7ea2307cc6f ''Nuclear fusion, pages 186-187, Gateway GCSE Physics, Oxford, OCR '']

← Older revision		Revision as of 18:37, 23 November 2019
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	:[https://www.amazon.co.uk/gp/product/178294558X/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=178294558X&linkCode=as2&tag=nrjc-21&linkId=f0dfb66dafcb0c6e9449e7b1a4ae1ac339 ''Nuclear fusion, pages 49, 100, GCSE Physics; The Revision Guide, CGP, AQA '']		:[https://www.amazon.co.uk/gp/product/178294558X/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=178294558X&linkCode=as2&tag=nrjc-21&linkId=f0dfb66dafcb0c6e9449e7b1a4ae1ac339 ''Nuclear fusion, pages 49, 100, GCSE Physics; The Revision Guide, CGP, AQA '']
	:[https://www.amazon.co.uk/gp/product/1471851370/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1471851370&linkCode=as2&tag=nrjc-21&linkId=01c69b0ae058f809cf636033e6ba793e ''Nuclear fusion; in stars, page 252, GCSE Physics, Hodder, AQA '']		:[https://www.amazon.co.uk/gp/product/1471851370/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1471851370&linkCode=as2&tag=nrjc-21&linkId=01c69b0ae058f809cf636033e6ba793e ''Nuclear fusion; in stars, page 252, GCSE Physics, Hodder, AQA '']
		+
		+	====Edexcel====
		+
		+	:[https://www.amazon.co.uk/gp/product/1782945733/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1782945733&linkCode=as2&tag=nrjc-21&linkId=2a2dbec9db6bf5766c0458d908fa0a52 ''Nuclear fusion, page 58, GCSE Physics; The Revision Guide, CGP, Edexcel '']
		+	:[https://www.amazon.co.uk/gp/product/1292120223/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1292120223&linkCode=as2&tag=nrjc-21&linkId=068ecf40278c32406a7f1c6e66751417 ''Nuclear fusion, pages 110, 114-115, GCSE Physics, Pearson Edexcel '']

← Older revision		Revision as of 14:40, 10 November 2019
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	<math>{}_1^1H + {}_1^3H \rightarrow {}_2^4He</math>		<math>{}_1^1H + {}_1^3H \rightarrow {}_2^4He</math>
	\|}		\|}
		+
		+	===References===
		+	====AQA====
		+
		+	:[https://www.amazon.co.uk/gp/product/1471851370/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1471851370&linkCode=as2&tag=nrjc-21&linkId=01c69b0ae058f809cf636033e6ba793e ''Nuclear fusion, page 108, GCSE Physics, Hodder, AQA '']
		+	:[https://www.amazon.co.uk/gp/product/1471851346/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1471851346&linkCode=as2&tag=nrjc-21&linkId=3ac654f4b0da781c49c855a1af4c92ea ''Nuclear fusion, page 244, GCSE Chemistry, Hodder, AQA '']
		+	:[https://www.amazon.co.uk/gp/product/019835939X/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=019835939X&linkCode=as2&tag=nrjc-21&linkId=57e96876985fc39b1a3d8a3e3dc238b6 ''Nuclear fusion, pages 106-107, GCSE Physics; Third Edition, Oxford University Press, AQA '']
		+	:[https://www.amazon.co.uk/gp/product/1782945970/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1782945970&linkCode=as2&tag=nrjc-21&linkId=a120d24dcc7cc7a58192069a3aafc1d2 ''Nuclear fusion, pages 140, 141, 318, GCSE Physics; The Complete 9-1 Course for AQA, CGP, AQA '']
		+	:[https://www.amazon.co.uk/gp/product/1471851362/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1471851362&linkCode=as2&tag=nrjc-21&linkId=7d78d70a2044ee9982dae010c94af92a ''Nuclear fusion, pages 187-8, GCSE Combined Science Trilogy 2, Hodder, AQA '']
		+	:[https://www.amazon.co.uk/gp/product/178294558X/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=178294558X&linkCode=as2&tag=nrjc-21&linkId=f0dfb66dafcb0c6e9449e7b1a4ae1ac339 ''Nuclear fusion, pages 49, 100, GCSE Physics; The Revision Guide, CGP, AQA '']
		+	:[https://www.amazon.co.uk/gp/product/1471851370/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1471851370&linkCode=as2&tag=nrjc-21&linkId=01c69b0ae058f809cf636033e6ba793e ''Nuclear fusion; in stars, page 252, GCSE Physics, Hodder, AQA '']

@@ Line 4: / Line 4: @@
 ===About Nuclear Fusion===
-: In a '''nuclear fusion reaction''' the products have less [[mass]] than the reactants as some of the [[Rest Mass Energy|rest mass]] is converted into [[energy]] in the process.
+: In a '''nuclear fusion reaction''' the products have less [[mass]] than the reactants as some of the [[mass]] is converted into [[energy]] in the process due to the [[Mass-Energy Equivalence]].
 : For a '''fusion''' [[Nuclear Reaction|reaction]] to occur the two [[Atomic Nucleus|nuclei]] must have enough [[Kinetic Energy Store|kinetic energy]] to overcome the [[Electrostatic Force|electrostatic force]] of repulsion between the [[Positive Charge|positively charged]] [[Atomic Nucleus|nuclei]].
 : To provide enough [[Kinetic Energy Store|kinetic energy]] to the [[Atomic Nucleus|nuclei]] the [[substance]] must be [[heat]]ed to a [[temperature]] of several million [[Degrees Celsius|degrees Celsius]].

@@ Line 6: / Line 6: @@
 : In a '''nuclear fusion reaction''' the products have less [[mass]] than the reactants as some of the [[Rest Mass Energy|rest mass]] is converted into [[energy]] in the process.
 : For a '''fusion''' [[Nuclear Reaction|reaction]] to occur the two [[Atomic Nucleus|nuclei]] must have enough [[Kinetic Energy Store|kinetic energy]] to overcome the [[Electrostatic Force|electrostatic force]] of repulsion between the [[Positive Charge|positively charged]] [[Atomic Nucleus|nuclei]].
-: To provide enough [[Kinetic Energy Store|kinetic energy]] to the [[Atomic Nuclei|nuclei]] the [[substance]] must be [[heat]]ed to a [[temperature]] of several million [[Degrees Celsius|degrees Celsius]].
+: To provide enough [[Kinetic Energy Store|kinetic energy]] to the [[Atomic Nucleus|nuclei]] the [[substance]] must be [[heat]]ed to a [[temperature]] of several million [[Degrees Celsius|degrees Celsius]].
 : '''Nuclear fusion''' occurs naturally in the centre of a [[Star]] due to the high [[temperature]]s and [[pressure]].
 : '''Nuclear fusion''' is possible in [[laboratory|laboratories]] on [[Earth]] but it cannot be sustained for long periods of [[time]] to produce enough [[energy]] to be useful as an [[Energy Resource|energy resource]].

@@ Line 10: / Line 10: @@
 : '''Nuclear fusion''' in [[laboratory|laboratories]] on [[Earth]] must be done at much higher [[temperature]] than in the centre of [[Star]]s because the centre of [[Star]]s is a much higher [[pressure]] so [[Atomic Nucleus|nuclei]] collide more often.
 {| class="wikitable"
 |-

@@ Line 12: / Line 12: @@
 {| class="wikitable"
 |-
-|[[File:FusionDTH.png|center|500px]]
+|[[File:FusionTDH.png|center|500px]]
 |-
 | style="height:20px; width:500px; text-align:center;" |'''Fusion''' of a [[Tritium]] and a [[Deuterium]] [[Atomic Nucleus|nucleus]] produces a [[Helium]] [[Atomic Nucleus|nucleus]].