The wormhole

A tunnel through space with a mouth at each end. Morris and Thorne worked out what it takes to walk through one and live: a throat hundreds of kilometres wide, held open by matter that weighs less than nothing. Then they noticed that one trip with a mouth turns it into a time machine.

the tunnel surface the throat the traveller and the one-g limit

Controls

The picture is an embedding diagram: one slice through the tunnel, drawn as a surface so you can see its shape. Up and down are not directions in space, only a way of showing how the tunnel narrows to the throat and opens out again on the far side. The dashed ring is how wide the throat has to be for a person to pass at this speed and feel no more than one g of tidal stretch.

Things to notice

The throat bound grows with speed

In the throat view set the speed to 0.01c. The dashed one-g ring sits at 1,000 km for the Ellis tunnel and at 500 km if you switch to Morris and Thorne's own shape, the register's number. Slide the speed to 0.1c and both grow tenfold. The ring scales as γv.

Register HAZ-3

Bigger is safer and dearer

Slide the throat radius up. The tension at the throat falls, but the mass of negative-energy matter needed to hold it open grows in step with the radius: about 170 suns' worth at 500 km, about 3,400 at 10,000 km.

Register STA-2

One trip makes a time machine

Switch to the time machine, set 0.9c and one year. Mouth B comes home 0.56 years younger than mouth A, and the tunnel now leads 0.56 years into the past. Nothing on the diagram ever moves faster than light.

Register CAU-3

Watch the clocks drift apart

In the time machine view press play. Mouth B climbs its V on the diagram while A's dial turns at the home rate and B's at 1/γ of it, so the gap between the two readings opens on the way out and keeps opening on the way home. When B lands the crossing arrow appears, and its height is the lag the two dials now show.

Why no FTL is needed

The twin paradox does all the work

Push the trip speed toward 0.95c: the offset climbs toward 69 percent of the trip time. The whole effect is ordinary time dilation plus a tunnel that keeps the two clocks in step. That is why every wormhole owes this bill.

Why no FTL is needed

The conjectured stop

Hawking's chronology protection: as the loop is about to close, the energy of quantum fields piles up on the edge of the time-travel region and the back reaction shuts it. Set any offset you like on the diagram; this is the claim that the last step never happens. A conjecture, not a theorem.

Register CAU-2

It cannot be a shortcut at all

Topological censorship: if the averaged null energy condition holds, no wormhole beats the outside route. The tunnel drawn here is a shortcut, so it needs a violation no known field supplies. The modern traversable wormholes obey the theorem by being long, and the time-machine step fails on them.

Register ENE-7

What is going on

Morris and Thorne, in 1988, wrote down the tunnel a traveller would want, a throat with no horizon and gentle tides, and asked Einstein's equations what would have to be inside it. The answer is matter with negative energy density along the light rays that thread the throat, which they called exotic matter. Nothing known supplies it, and the amount grows with the size of the throat. That is STA-2 in the register. The size of the throat is set by comfort: one Earth g of tidal stretch across a two-metre body, which bounds the tidal terms at the throat by about (108 m)-2 and gives a throat radius that scales with the speed of the crossing, about 500 km at one percent of light speed for their design shape. That is HAZ-3.

Within the year, with Yurtsever, they showed that any such wormhole is a time machine with an assembly step: carry one mouth away at high speed and bring it back, and its clock lags the other by T(1 − 1/γ), while the tunnel still joins the mouths at equal clock readings. Walk in at the mouth that travelled and you step out of the other one in the past. That is CAU-3. Hawking's reply in 1992, chronology protection, CAU-2, conjectures that quantum back reaction stops the loop from ever closing. And a theorem of Friedman, Schleich and Witt from 1993, with the averaged null energy condition proved for the geodesics it needs between 2007 and 2017, says a wormhole in ordinary flat surroundings cannot be a shortcut at all: that is topological censorship, ENE-7. The traversable wormholes built since 2017 by Gao, Jafferis and Wall and by Maldacena, Milekhin and Popov obey it by being longer inside than the way round, which is also why they cannot be turned into time machines.