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arxiv: 1002.3876 · v2 · submitted 2010-02-20 · ✦ hep-th · gr-qc· quant-ph

Comments on "On the Origin of Gravity and the Laws of Newton", by Erik Verlinde

classification ✦ hep-th gr-qcquant-ph
keywords screenverlindeaccelerationdeltaholographichorizonviewedaccordance
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We argue that the relativistic Unruh temperature cannot be associated with the bits on the screen, in the form considered by Verlinde. The acceleration $a$ is a scalar quantity (the modulus of the acceleration four vecor) and not a vector. When the mass $m$ approaches the holographic screen, viewed as a stretched horizon, the shift $\Delta x$ from Verlinde's Eq. (3.15) becomes $c^{2}/a$ and the entropy variation equals $(1/2) k_{B} \Delta N$, in accordance with Gao's calculations. Using the Heisenberg Principle we show that the energy on the causal horizon (viewed as a holographic screen) of an inertial observer is proportional to its radius, as for a black hole.

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