All the Standard Model particles were discovered well below the energy scale of approximately 10¹² eV or 1 TeV. The heaviest Standard Model particle is the top quark, with a mass of approximately 173 GeV.

Above these energies, desert theory predicts no particles will be discovered until reaching the scale of approximately 10²⁵ eV^[why?]. According to the theory, measurements of TeV-scale physics at the Large Hadron Collider (LHC) and the near-future International Linear Collider (ILC) will allow extrapolation all the way up to the GUT scale ^{[citation needed]}.

The particle desert's negative implication is that experimental physics will simply have nothing more fundamental to discover, over a very long period of time. Depending on the rate of the increase in experiment energies, this period might be a hundred years or more. Presumably, even if the energy achieved in the LHC, ~ 10¹³ eV, were increased by up to 12 orders of magnitude, this would only result in producing more copious amounts of the particles known today, with no underlying structure being probed. The aforementioned timespan might be shortened by observing the GUT scale through a radical development in accelerator physics, or by a non-accelerator observational technology, such as examining tremendously high energy cosmic ray events, or another, yet undeveloped technology.

Alternatives to the desert exhibit particles and interactions unfolding with every few orders of magnitude increase in the energy scale.

With the Minimal Supersymmetric Standard Model, adjustment of parameters can make the grand unification exact. This unification is not unique.

Such exact gauge unification is a generic feature of supersymmetric models, and remains a major theoretical motivation for developing them. Such models automatically introduce new particles ("superpartners") at a new energy scale associated with the breaking of the new symmetry, ruling out the conventional energy desert. They can, however, contain an analogous "desert" between the new energy scale and the GUT scale.

Scenarios like the Katoptron model can also lead to exact unification after a similar energetic desert. If the known neutrino masses are due to a seesaw mechanism, the new heavy neutrino states must have masses below the GUT scale in order to produce the observed O(1 meV) masses. Indicative examples of the order of magnitude of the corresponding masses and fermion mixing parameters in accordance with experimental data have been calculated within the context of katoptrons.^[1][2]

As of 2019, the LHC has excluded the existence of many new particles up to masses of a few TeV, or about 10x the mass of the top quark. Other indirect evidence in favor of a large energy desert for a certain distance above the electroweak scale (or even no particles at all beyond this scale) includes:

1. The absence of any observed proton decays, which has already ruled out many new physics models that can produce them up to (and beyond) the GUT scale. ^{[citation needed]}
2. Precision measurements of known particles and processes, such as extremely rare particle decays, have already indirectly probed energy scales up to 1 PeV (10⁶ GeV) without finding any confirmed deviations from the Standard Model. This significantly constrains any new physics that might exist below those energies.
3. Research from experimental data on the cosmological constant, LIGO noise, and pulsar timing, suggests it's very unlikely that there are any new particles with masses much higher than those which can be found in the standard model or the Large Hadron Collider.^[3][4][5] However, this research has also indicated that quantum gravity or perturbative quantum field theory will become strongly coupled before 1 PeV, leading to other new physics in the TeVs.^[3]
4. The observed Higgs boson decay modes and rates are so far consistent with the Standard Model.

So far there is no direct evidence of new fundamental particles with masses between the electroweak and GUT scale, consistent with the desert. However, there are some theories about why such particles might exist:

1. The leading theoretical explanations of neutrino masses, the various seesaw models, all require new heavy neutrino states below the GUT scale.
2. Both weakly interacting massive particles (WIMP) and axion models for dark matter require the new, long-lived particles to have masses far below the GUT scale.
3. In the Standard Model, there is no physics which stabilizes the Higgs boson mass to its actual observed value. Since the actual value is far below the GUT scale, whatever new physics ultimately does stabilize it must become apparent at lower energies too.
4. Precision measurements have produced several outstanding discrepancies with the Standard Model in recent years. These include anomalies in certain B meson decays and a discrepancy in the measured value of the Muon g-2 (anomalous magnetic moment). Depending on the results of currently ongoing experiments, these effects may already indicate the existence of unknown new particles below about 100 TeV.

• Wolchover, Natalie (9 August 2016). "What No New Particles Means for Physics". Quanta Magazine. Simons Foundation. Retrieved 19 December 2016.
• Dimopoulos, Savas (1990). "LHC, SSC and the universe". Physics Letters B. 246 (3–4): 347–352. Bibcode:1990PhLB..246..347D. doi:10.1016/0370-2693(90)90612-A.
• Kawamura, Yoshiharu; Kinami, Teppei; Miura, Takashi (2009). "Superparticle sum rules in the presence of hidden sector dynamics". Journal of High Energy Physics. 2009 (1): 064. arXiv:0810.3965. Bibcode:2009JHEP...01..064K. doi:10.1088/1126-6708/2009/01/064.