One finds a useful definition for enthalpy ##H## in the book “Introduction to Thermal Physics” by Daniel V. Schroeder:
Enthalpy
Constant-pressure processes occur quite often, both in the natural world and in the laboratory. Keeping track of the compression-expansion work done during these processes gets to be a pain after a while, but there is a convenient trick that makes it a bit easier. Instead of always talking about the energy content of a system, we can agree to always add in the work needed to make room for it (under a constant pressure, usually 1 atm). This work is ##PV##, the pressure of the environment times the total volume of the system (that is, the total space you would need to clear out to make room for it). Adding ##PV## onto the energy gives a quantity called the enthalpy, denoted ##H##:
$$H\equiv U + PV.$$
This is the total energy you would have to come up with, to create the system out of nothing and put it into the environment (see Figure 1.15). Or, put another way, if you could somehow annihilate the system, the energy you could extract is not just ##U##, but also the work ##(PV)## done by the atmosphere as it collapses to fill the vacuum left behind.