Hawking shows that black holes radiate
node
Applying quantum field theory to the curved spacetime around a horizon, Stephen Hawking found that a black hole emits a thermal spectrum at a temperature inversely proportional to its mass, and published the result in Nature under the title "Black hole explosions?". The calculation vindicated Bekenstein's entropy proposal and fixed its coefficient, and it made black holes objects that lose mass and can in principle disappear. For every known astrophysical black hole the predicted temperature is far below that of the cosmic microwave background, so the effect has never been observed.
A node is not a place. Drawing it on a map would assert something about the world that no stored fact supports.
Read in · 1
Evidence · 1
Timeline
No dated observations are stored for this object. Atlas shows what was observed and when — it does not infer a history.
Connections · 3
- Hawking radiationconcerns
- Stephen Hawkingconcerns
- Black hole entropyconcerns
Assembled narrative · 1
Assembled from 30 blocks · 1 evidence · 15 related
- Story
- Applying quantum field theory to the curved spacetime around a horizon, Stephen Hawking found that a black hole emits a thermal spectrum at a temperature inversely proportional to its mass, and published the result in Nature under the title "Black hole explosions?". The calculation vindicated Bekenstein's entropy proposal and fixed its coefficient, and it made black holes objects that lose mass and can in principle disappear. For every known astrophysical black hole the predicted temperature is far below that of the cosmic microwave background, so the effect has never been observed.
- Knowledge
- Hawking radiation
- Black hole entropy
- Stephen Hawking
- Hawking shows that black holes radiate
- Connections
- Hawking radiation
- Stephen Hawking
- Black hole entropy
- Stephen Hawking
- Black hole entropy
- The black hole information paradox
- Hawking shows that black holes radiate
- Hawking argues that information is destroyed
- The Page curve is reproduced from within semiclassical gravity
- Hawking radiation
- Hawking shows that black holes radiate
- Hawking argues that information is destroyed
- Hawking concedes the information bet
- The event horizon
- Jacob Bekenstein
- Hawking radiation
- Bekenstein assigns entropy to a black hole
- Hawking shows that black holes radiate
- Page states what unitarity requires of the radiation
- The Page curve is reproduced from within semiclassical gravity
- Evidence
- Derives thermal emission from a black hole horizon at a temperature inversely proportional to mass. V55 VERIFICATION BASIS: not consulted in session; no research tool was available. Volume and page are from recall of a canonical citation and must be checked. The fuller treatment appeared in Communications in Mathematical Physics in 1975 and is deliberately not cited by volume here.
Observed changes · 0
No public Signals are attached to this object. Signals show what changed and when it was observed — never a direction or a rank.
Actions
/atlas?object=EVT_HAWKING_RADIATION_1974&experience=EVT_HAWKING_RADIATION_1974