Church–Turing thesis — defines the boundary of what is computable
Completeness
Computable — can be solved by a Turing machine
Consistent — no contradictions in the system
Decidable — algorithm exists that always halts with yes/no
Vocabulary
Entscheidungsproblem - Ent-shy-dungs-problem - decision problem posed by Hilbert
Finite — limited in size or length
Halting Problem — classic undecidable problem
Paradox — self-contradictory result (like Russell’s Paradox or the Liar Paradox)
Turing machine — model of computation
Undecidable — no such algorithm exists
The Players
David Hilbert (1862–1943)
German mathematician. University of Göttingen in Germany.
Wilhelm Ackermann (1896–1962)
Student and collaborator of Hilbert. University of Göttingen in Germany.
Alonzo Church (1903–1995)
American logician. Princeton University in the USA.
Alan Turing (1912–1954)
British mathematician and founder of computer science. University of Cambridge (UK).
From 1936 to 1938, Turing went to Princeton to do his PhD under Alonzo Church.
Timeline of Publications
1928 Hilbert and Ackermann Grundzüge der theoretischen Logik (Principles of Mathematical Logic).
They formalised first-order logic and clearly defined the Entscheidungsproblem (decision problem): whether there exists a general mechanical procedure (algorithm) to decide if any given statement is provable.
Timeline of Publications
1936 Alonzo Church “An Unsolvable Problem of Elementary Number Theory” published.
Church used lambda calculus to prove that the Entscheidungsproblem is undecidable — showing that there is no general algorithm to decide provability for all statements in first-order logic.
Timeline of Publications
1936 Alan Turing “On Computable Numbers, with an Application to the Entscheidungsproblem” published.
Turing introduced the Turing machine as a new model of computation.
He proved the Halting Problem is undecidable, which implies that the Entscheidungsproblem is undecidable too.
The Story
In the early 20th century, mathematics faced a crisis due to logical paradoxes, such as Russell’s Paradox.
Hilbert proposed a solution: formalise all of mathematics using a set of axioms and rules. His goal was a symbolic system in which all mathematical truths could be derived mechanically — no intuition, just logic.
The Story
Ackermann worked with Hilbert to formalise logic and pose the Entscheidungsproblem: to find a single algorithm that could decide if a mathematical statement was true or false.
In 1936, Alonzo Church proved that the Entscheidungsproblem is undecidable, using a formal model of computation called lambda calculus.
The Story
Around the same time, Alan Turing independently proved the same result using his new model of computation — the Turing machine — by showing that the Halting Problem is undecidable.
Church and Turing’s work led to the formulation of the Church–Turing Thesis, the formal limit of what can be computed.
Some Details
Hilbert’s Program
Hilbert’s program aimed to reduce all of mathematics to formal symbolic manipulations.
Every line follows strictly from axioms and rules:
No intuition, no diagrams, no external meanings.
Just symbols and logic.
Hilbert’s Program
In his 1927 program to fully formalise mathematical reasoning, David Hilbert outlined the following three goals:
Mathematics should be complete: all true mathematical statements can be derived from a finite set of axioms.
Mathematics should be consistent: no contradictions.
Mathematics should be decidable: proofs can be verified by a single algorithm.
Example – not on study design
Peano and Addition Axioms
( 0 ) Zero is a natural number.
( x , S(x) ) Every natural number has a successor.
( x , S(x) ) Zero is not the successor of any number.
( x, y , S(x) = S(y) x = y ) The successor function is injective (no two numbers share a successor).
( x , x + 0 = x ) Zero is the additive identity.
( x, y , x + S(y) = S(x + y) ) Defines addition recursively using the successor function.
Classic physics as Example
The finite set of axioms: Newton’s three laws of motion and the Law of Universal Gravitation.
Key equations:
\[
\text{Newton's Second Law:} \quad F = ma
\]
\[
\text{Law of Universal Gravitation:} \quad F = G \frac{m_1 m_2}{r^2}
\]
Classic physics as Example
From just these axioms, you can:
Predict the orbit of Earth around the Sun (Kepler’s laws).
Calculate the trajectory of a rocket.
Explain phenomena like tides.
Classic physics as Example
The laws act like a formal system:
They are finite (a few basic laws).
They are consistent (no contradictions).
They are decidable for simple systems (you can solve the equations exactly).
Where Limits Appear
However, as systems become more complex:
Many-body problems become chaotic.
Exact solutions may be impossible; only approximations exist.